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Exoplanet astronomy
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Galactic and extragalactic astronomy
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-Galaxies
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---D galaxies
----cD galaxies
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---LINER galaxies
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---Seyfert galaxies
--Field galaxies
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---Brightest cluster galaxies
---cD galaxies
---Giant elliptical galaxies
--High-redshift galaxies
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--Infrared excess galaxies
--Interacting galaxies
---Galaxy collisions
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--Irregular galaxies
---Amorphous irregular galaxies
---Dwarf irregular galaxies
---I galaxies
---Magellanic Clouds
----Large Magellanic Cloud
----Magellanic Stream
----Small Magellanic Cloud
--Late-type galaxies
--Low surface brightness galaxies
---L galaxies
--Lyman-alpha galaxies
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--Primordial galaxies
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-Galaxy clusters
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--Intracluster medium
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--Virgo Cluster
-Galaxy groups
--Hickson compact group
--Local Group
---Andromeda Galaxy
---Magellanic Clouds
----Large Magellanic Cloud
----Magellanic Stream
----Small Magellanic Cloud
---Milky Way Galaxy
---Triangulum Galaxy
--Seyfert's sextant
--Stefan's quintet
-Galaxy physics
--Galactic accretion disks
--Galaxy abundances
--Galaxy cluster counts
--Galaxy distances
---Holmberg radius
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--Galaxy dynamics
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---Density wave model
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----Galaxy infall
---Galaxy dynamics
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----Galaxy chemical evolution
-----Chemical enrichment
---Galaxy kinematics
----Galaxy anticenters
----Galaxy equators
----Galaxy planes
----Galaxy rotation
-----Galaxy rotation curves
-----Oort constants
---Galaxy winds
--Galaxy properties
---Galaxy ages
---Galaxy chemical composition
---Galaxy colors
----Blue cloud galaxies
----Green valley galaxies
----Red sequence galaxies
---Galaxy fountains
---Galaxy jets
---Galaxy luminosities
---Galaxy magnetic fields
---Galaxy magnitudes
---Galaxy masses
----Galaxy mass distribution
-----Navarro-Frenk-White profile
---Galaxy radial velocities
---Galaxy radii
---Galaxy stellar content
--Galaxy spurs
--Galaxy structure
---Galaxy components
----Galaxy bulges
----Galaxy disks
-----Stellar disks
----Galaxy halos
-----Stellar rings
----Galaxy nuclei
-----Active galactic nuclei
------Blazars
------Quasars
-------Broad-absorption line quasar
-------Double quasars
-------Individual quasars
-------Quasar-galaxy pairs
-------Radio loud quasars
-------Radio quiet quasars
-------X-ray quasars
------Radio cores
------Radio hot spots
------Radio jets
-------Polar jets
-------Relativistic jets
------Radio lobes
------Radio plumes
------Relativistic disks
-----Galaxy circumnuclear disk
----Spiral arms
----Tidal tails
---Radio cores
---Spiral pitch angle
--Galaxy voids
--Milky Way Galaxy physics
---Galactic anticenter
---Galactic center
---Galactic winds
---Gould Belt
---Milk Way dark matter halo
---Milky Way disk
---Milky Way dynamics
---Milky Way evolution
---Milky Way formation
---Milky Way Galaxy fountains
---Milky Way magnetic fields
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---Milky Way stellar halo
---Solar neighborhood
--Stellar kinematics
---Stellar motion
----Proper motions
High energy astrophysics
-Active galactic nuclei
--Blazars
--Quasars
---Broad-absorption line quasar
---Double quasars
---Individual quasars
---Quasar-galaxy pairs
---Radio loud quasars
---Radio quiet quasars
---X-ray quasars
--Radio cores
--Radio hot spots
--Radio jets
---Polar jets
---Relativistic jets
--Radio lobes
--Radio plumes
--Relativistic disks
-Astroparticle physics
--Cosmic rays
---Cosmic ray showers
---Cosmic ray sources
---Forbush effect
---Galactic cosmic rays
---High-energy cosmic radiation
---Secondary cosmic rays
---Ultra-high-energy cosmic radiation
--Cosmological neutrinos
--Gamma rays
---Gamma-ray lines
---Gamma-ray sources
----Soft gamma ray repeaters
--Gravitational waves
---Gravitational wave sources
---pp waves
--Neutrino oscillations
--Solar neutrinos
--Supernova neutrinos
--Urca process
-Black hole physics
--Bekenstein–Hawking entropy
--Black hole spin-flip
--Black hole thermodynamics
--Ergosphere
--Event horizons
--Hawking radiation
--Kruskal diagram
--Penrose process
--Photon sphere
--Quasinormal modes
--Trans-Planckian physics
-Black holes
--Astrophysical black holes
---Intermediate-mass black holes
---Primordial black holes
---Stellar mass black holes
---Supermassive black holes
----Quasars
-----Broad-absorption line quasar
-----Double quasars
-----Individual quasars
-----Quasar-galaxy pairs
-----Radio loud quasars
-----Radio quiet quasars
-----X-ray quasars
--Classical black holes
---Charged black holes
----Kerr-Newman black holes
----Reissner–Nordström black holes
---Nonrotating black holes
----Reissner–Nordström black holes
----Schwarzschild black holes
---Rotating black holes
----Kerr black holes
-----Maximal Kerr black holes
----Kerr-Newman black holes
---Uncharged black holes
----Kerr black holes
-----Maximal Kerr black holes
----Schwarzschild black holes
-Burst astrophysics
--Gamma-ray bursts
--Optical bursts
--Radio bursts
--Rapid bursts
--X-ray bursts
-Dark matter
--Baryonic dark matter
--Cold dark matter
--Hot dark matter
--Warm dark matter
-Intracluster medium
-Jets
--Galaxy jets
--Plasma jets
--Radio jets
---Polar jets
---Relativistic jets
--Stellar jets
-Neutrino astronomy
--Neutrino masses
--Solar neutrino problem
--Urca process
-Plasma astrophysics
--Cosmic electrodynamics
--Space plasmas
---Alfven waves
-Relativistic binary stars
-Seyfert galaxies
-Warm-hot intergalactic medium
Interdisciplinary astronomy
-Archaeoastronomy
--Ethnoastronomy
--Megalithic astronomy
-Astrobiology
--Exobiology
--Xenobiology
-Astrochemistry
--Chemical abundances
---Abundance ratio
---Cosmic abundance
---Frozen in elements
---Galaxy abundances
---Interstellar abundances
---Isotopic abundance
---Metal abundance
---Nuclear abundances
---Overabundance
---Stellar abundances
----Beryllium abundance
----Boron abundance
----Helium abundance
----Lithium abundance
---Underabundance
--CII region
--Cosmochemistry
--Diffuse interstellar bands
-Astrophysical fluid dynamics
--Hydrodynamical simulations
--Internal waves
-Molecular astrophysics
-Philosophy of astronomy
-Sociology of astronomy
Interstellar medium
-Astrophysical masers
--Hydroxyl masers
--Megamasers
--Silicon monoxide masers
--Water masers
-Intercloud medium
-Interstellar absorption
--Diffuse interstellar bands
--Interstellar dust extinction
--Interstellar line absorption
-Interstellar atomic gas
-Interstellar clouds
--Dark interstellar clouds
---Bok globules
---Cometary globules
---Infrared dark clouds
--Dense interstellar clouds
--Diffuse interstellar clouds
--Evaporating gaseous globules
--High-velocity clouds
---Magellanic Stream
--Interstellar dust
---Carbonaceous grains
---Polycyclic aromatic hydrocarbons
---Silicate grains
---Very small grains
--Molecular clouds
---Collapsing clouds
---Diffuse molecular clouds
---Giant molecular clouds
---Infrared dark clouds
---Photodissociation regions
--Neutral hydrogen clouds
--Plasma clouds
-Interstellar dynamics
-Interstellar emissions
--Continuum radio emission
--Dust continuum emission
--Interstellar cyclotron emission
--Interstellar line emission
---CO line emission
---H1 line emission
--Interstellar masers
--Interstellar synchrotron emission
--Interstellar thermal emission
-Interstellar filaments
-Interstellar magnetic fields
-Interstellar molecules
-Interstellar phases
--Cold neutral medium
--Hot ionized medium
--Molecular gas
--Warm ionized medium
--Warm neutral medium
-Interstellar plasma
-Interstellar radiation field
-Interstellar scattering
--Interstellar dust extinction
-Nebulae
--Bipolar nebulae
--Bright nebulae
--Cometary nebulae
--Compact nebulae
--Dark interstellar clouds
---Bok globules
---Cometary globules
---Infrared dark clouds
--Diffuse nebulae
--Dust nebulae
--Emission nebulae
---H II regions
----Bok globules
----Compact H II region
---Planetary nebulae
----Individual planetary nebulae
----Planetary nebulae nuclei
--Filamentary nebulae
--Gaseous nebulae
--H I regions
---HI shells
--Pre-solar nebulae
--Protoplanetary nebulae
--Reflection nebulae
--Ring nebulae
--Supernova remnants
-Protostars
--Bok globules
--Cocoon stars
--Cometary nebulae
--Proplyds
--Young stellar objects
---Pre-main sequence stars
----Herbig Ae/Be stars
----Herbig-Haro objects
----T Tauri stars
-----Classical T Tauri stars
-----FU Orionis stars
-----Weak-line T Tauri stars
-Stellar bridges
-Stellar wind bubbles
--Heliosphere
---Heliopause
---Heliosheath
---Stellar bow shocks
---Termination shock
-Stellar-interstellar interactions
--Astrospheres
--Interstellar medium wind
--Stellar jets
--Stellar winds
-Superbubbles
-Supernova remnants
-Tidal tails
Observational astronomy
-Astronomical research
--Amateur astronomers
--Analytical mathematics
---Astronomical models
----Burkert profile
----Gas-to-dust ratio
----Mass-to-light ratio
----Oort constants
----Star counts
---Luminosity function
---Perturbation methods
---Radiative transfer equation
---von Zeipel theorem
--Astronomers
--Astronomical reference materials
---Almanacs
----Nautical almanacs
---Astronomical databases
---Calendars
---Catalogs
----Astrographic catalogs
----Celestial objects catalogs
----FK catalog
----Henry Draper catalog
----Radio source catalogs
----Sky surveys
---Ephemerides
---Finding charts
---Finding lists
---Star atlases
---Surveys
----Galaxy counts
----Kapteyn Selected Areas
----Radio source counts
----Redshift surveys
----Sky surveys
----Star counts
----Ultraviolet surveys
----X-ray surveys
--Astronomical site protection
--Astrophysicists
--Classification systems
---Galaxy classification systems
----DDO classification
----De Vaucouleurs Sandage classification
----Hubble classification scheme
---Hertzsprung Russell diagrams
----Blue loop
----Giant branches
-----Red giant branch
------Red giant bump
------Red giant clump
------Red giant tip
----Hertzsprung gap
----Instability strip
----Post-asymptotic giant branch
----Turnoff point
---Luminosity classification
----Kappa mechanism
---Stellar classification
----Henry Draper Catalogue
----Yerkes classification
---Stellar evolutionary tracks
----Hayashi track
----Henyey track
--Sociology of astronomy
--Space research
---Microgravity
-Instrumentation
--Astronomical detectors
---CMBR detectors
---Cosmic ray detectors
---Dark matter detectors
---Gamma-ray detectors
---Gravitational wave detectors
---Radio receivers
---X-ray detectors
--Early astronomical instruments
---Armillary spheres
---Astronomical sextants
---Orreries
---Photoheliographs
---Ptolemy stones
---Stone circles
---Zenith tubes
--High altitude balloons
--Interferometers
---Fabry-Perot interferometers
---Mach-Zehnder interferometers
---Michelson interferometers
--Observatories
---Antarctic observatories
---Domes
---Gamma-ray observatories
---Infrared observatories
----Infrared Astronomical Satellite
---Optical observatories
----Hubble Space Telescope
---Radio observatories
---Solar observatories
---Space observatories
----Gamma-ray observatories
----Hubble Space Telescope
----Infrared Astronomical Satellite
---Ultraviolet observatories
----Hubble Space Telescope
---X-ray observatories
--Polarimeters
--Siderostats
--Solar instruments
--Space vehicles
---Artificial satellites
----Geosynchronous satellites
-----Geostationary satellites
---Hall thrusters
---Space debris
---Space probes
----Deep space probes
----Flyby missions
----Landers
----Lunar probes
----Orbiters
----Planetary probes
----Rovers
---Space vehicle instruments
----Space telescopes
-----Gamma-ray telescopes
-----Infrared telescopes
-----Ultraviolet telescopes
-----X-ray telescopes
--Spectrometers
---Mass spectrometers
--Stellar tracking devices
---Coelostats
---Heliostats
---Siderostats
--Telescopes
---Automated telescopes
----Automatic patrol telescopes
---Gamma ray telescopes
---Grazing incidence telescopes
---Ground telescopes
---Meridian circles
---Neutrino telescopes
---Optical telescopes
----Catadioptric telescopes
-----Baker-Nunn cameras
-----Bouwers telescope
-----Maksutov telescopes
-----Schmidt cameras
-----Schmidt-Cassegrain telescopes
----Multiple mirror telescope
----Reflecting telescopes
-----Cassegrain telescopes
------Ritchey–Chrétien telescopes
-----Gregorian telescopes
-----Newtonian telescopes
------Dobsonian telescopes
----Solar optical telescopes
----Very Large Telescope
---Radio telescopes
----Heterodyne receivers
----Radar telescopes
----Radio interferometers
-----Long baseline interferometers
-----Very Large Array
-----Very long baseline interferometers
----Radioheliographs
----Single-dish antennas
----Solar radio telescopes
---Solar telescopes
----Radioheliographs
----Solar optical telescopes
----Solar radio telescopes
---Space telescopes
----Gamma-ray telescopes
----Infrared telescopes
----Ultraviolet telescopes
----X-ray telescopes
---Telescope mounts
----Alt-azimuth mounts
----Equatorial mounts
-----English mounts
-----Fork mounts
-----German equatorial mounts
-----Horseshoe mounts
-----Yoke mounts
---Wide-field telescopes
----All-sky cameras
-----Cloud monitors
----Baker-Nunn cameras
--Transit instruments
---Meridian circles
---Zenith telescopes
---Zenith tubes
-Methods
--Amateur astronomy
---Night vision
---Purkinje effect
--Astrophotography
---Darkrooms
---Remote telescope astrophotography
---Telescope focal plane photography
--Computational astronomy
---Astroinformatics
---Astronomical databases
---Virtual observatories
--Cosmic ray astronomy
--Gamma-ray astronomy
--Gravitational wave astronomy
--Ground-based astronomy
--Infrared astronomy
---Far infrared astronomy
---Infrared excess
---Near infrared astronomy
--Neutrino astronomy
---Neutrino masses
---Solar neutrino problem
---Urca process
--Observational cosmology
---Cosmological constant
----Cosmological constant experiments
---Hubble constant
--Radio astronomy
---Brightness temperature
---Cosmic noise
----Cosmic microwave background radiation
-----Cosmic anisotropy
-----Cosmic isotropy
---Interplanetary scintillation
---Interstellar scintillation
---Millimeter astronomy
---Radio astrometry
---Radio spectroscopy
---Spectral index
---Submillimeter astronomy
---Sunyaev-Zeldovich effect
--Ultraviolet astronomy
---Near ultraviolet astronomy
--Visible astronomy
--Visual observation
---Limb brightening
---Limb darkening
---Optical doubles
---Optical identification
---Zenith hourly rate
--X-ray astronomy
---X-ray bright point
---X-ray identification
-Techniques
--Astrometry
---Astronomical coordinate systems
----Ecliptic coordinate system
-----Ecliptic latitude
-----Ecliptic longitude
-----Ecliptic poles
------North ecliptic pole
------South ecliptic pole
----Equatorial coordinate system
-----Celestial equator
-----Celestial poles
------North celestial pole
------South celestial pole
-----Celestial sphere
------Constellations
-----Declination
-----Equatorial zone
-----Equinox
------Autumnal equinox
------Vernal equinox
-----Equinox correction
-----Hour angle
-----Right ascension
-----Solstice
------Summer solstice
------Winter solstice
----Galactic coordinate system
-----Galactic latitude
-----Galactic longitude
-----Galactic poles
------North galactic pole
------South galactic pole
-----Quadrants
----Horizontal coordinate system
-----Altitude angle
-----Azimuth
-----Meridian
-----Nadir
-----Vertical circle
-----Zenith
----Supergalactic coordinate system
-----Supergalactic latitude
-----Supergalactic longitude
---Astronomical location
----Angular separation
----Apparent position
----Conjunction
----Line of sight
----Opposition
----Optical position
----True position
---Baade-Wesselink method
---Bolometric correction
---Brightness temperature
---Distance measure
----Astronomical unit
----Light year
----Parsec
---Effective temperature
---Equator position
---Fundamental parameters of stars
---Magnitude
----Absolute magnitude
-----Wilson-Bappu Effect
----Apparent magnitude
-----Limiting magnitude
-----Period determination
-----Photoelectric magnitude
-----Photographic magnitude
-----Photovisual magnitude
-----Pogson scale
-----Two-color diagrams
-----Variable star period change
----Integrated magnitude
---Parallax
----Annual parallax
----Diurnal parallax
-----Horizontal parallax
----Dynamical parallax
----Kinematic parallax
----Moving cluster parallax
----Photometric parallax
----Secular parallax
----Statistical parallax
----Stellar parallax
-----Solar parallax
----Trigonometric parallax
---Phase angle
---Phase defect
---Phase effect
---Phase error
---Photographic astrometry
----Photogrammetry
---Radial velocity
---Radio astrometry
---Relativistic aberration
---Relaxation time
---Sky noise
---Solar constant
---Space astrometry
---Spectral index
---Standard stars
----Comparison stars
----Photometric standard stars
---Stellar distance
----Cepheid distance
----Distance indicators
----Faber-Jackson distance
----Standard candles
---Syzygy
----Eclipses
-----Antumbra
-----Baily's beads
-----Lunar eclipses
------Saros cycle
-----Partial eclipses
-----Penumbra
-----Solar eclipses
------Diamond ring effect
------Flash spectra
------Shadow bands
-----Total eclipses
-----Umbra
-----Zone of totality
----Occultation
-----Annular eclipses
-----Asteroid occultation
-----Lunar occultation
-----Occulting disks
-----Radio occultation
----Transits
---Two-color diagrams
---Wolf diagram
--Astronomical object identification
--Astronomical optics
---Astronomical seeing
---Atmospheric refraction
---Atmospheric scintillation
----Ionospheric scintillation
---Collimation
---Dark adaption
---Extinction
----Atmospheric extinction
-----Ultraviolet extinction
----Interstellar extinction
-----Interstellar reddening
-----Reddened stars
----Reddening law
---Interplanetary scintillation
---Interstellar scintillation
---Laser guide stars
---Stellar atmospheric opacity
--CCD observation
--Coronographic imaging
--Doppler imaging
---Zeeman–Doppler imaging
--Doppler shift
---Blueshifted
---Redshifted
--Drift scan imaging
--Field of view
---Blank field
---High latitude field
---Parallel field
--High time resolution astrophysics
--Interferometry
---Adaptive interferometry
---Aperture synthesis
---Atom interferometry
---Direct detection interferometry
---Heterodyne interferometry
---Holographic interferometry
---Interferometric correlation
---Laser interferometry
----LIGO
---Long baseline interferometry
---Neutron interferometry
---Nonclassical interferometry
---Optical interferometry
----Optical phase shifting interferometry
-----Mach-Zehnder interferometers
-----Michelson interferometry
---Phase switching
---Radio interferometry
----Very long baseline interferometry
---Speckle interferometry
---Visibility function
--Optical observation
--Photometry
---CCD photometry
---Galaxy photometry
---Light curves
---Photoelectric photometry
---Photographic photometry
----Photogrammetry
---Photometric standard stars
---Photometric systems
----Broad band photometry
-----Bessel photometry
-----BV photometry
-----Cape photometry
-----Cape RI photometry
-----Gunn photometry
-----HST photometry
-----Johnson photometry
-----Kron-Cousins photometry
-----RGB photometry
-----RGU photometry
-----Sloan photometry
----Color equations
----Medium band photometry
-----DDO photometry
-----Geneva photometry
-----Strömgren photometric system
-----Vilnius photometry
-----Walraven photometry
----Multi-color photometry
----Narrow band photometry
-----H alpha photometry
-----H beta photometry
---Spectrophotometry
----Flux calibration
----Spectrophotometric standards
---Stellar photometry
---Surface photometry
---Two-color diagrams
---Waveband photometry
----Infrared photometry
----Ultraviolet photometry
-----Ultraviolet color
----X-ray photometry
-----Hardness ratio
--Pointing accuracy
---Pointing error
--Polarimetry
---Polarimetry [Exoplanets]
--Spectroscopy
---Lyman alpha forest
Solar astronomy
-CNO anomaly
-Helioseismology
--Helioseismic pulsations
--Solar cycle
---Active sun
---Quiet sun
---Sunspot cycle
--Solar magnetic fields
---Solar magnetic reconnection
-Solar abundances
-Solar activity
--Solar flares
---Radio flares
---X-ray flares
--Solar prominences
---Quiescent prominence
--Solar storm
--Sunspots
---Ephemeral active regions
---Maunder minimum
---Penumbral filaments
---Sunspot groups
----Bipolar sunspot groups
---Sunspot number
---Wilson effect
-Solar atmosphere
--Solar chromosphere
---Plages
--Solar corona
---M region
---Solar coronal holes
---Solar coronal loops
---Solar coronal streamers
---Solar transition region
--Solar photosphere
-Solar electromagnetic emission
--Solar extreme ultraviolet emission
--Solar gamma ray emission
--Solar radio emission
--Solar ultraviolet emission
--Solar X-ray emission
-Solar evolution
--Solar nebulae
-Solar faculae
-Solar filaments
-Solar flares
--Radio flares
--X-ray flares
-Solar granulation
--Mesogranulation
--Supergranulation
-Solar interior
--Solar core
-Solar motion
--Antapex
--Apex
--Solar atmospheric motions
-Solar oscillations
-Solar particle emission
--Solar energetic particles
--Solar neutrons
-Solar properties
--Solar composition
--Solar diameter
--Solar irradiance
--Solar magnetic fields
---Solar magnetic reconnection
--Solar magnetism
--Solar mass
--Solar rotation
-Solar radiation
--Diffuse radiation
-Solar rotation
-Solar spicules
--Fibrils
--Mottles
--Solar macrospicules
-Solar surface
-Solar wind
--Heliopause
-Sunspots
--Ephemeral active regions
--Maunder minimum
--Penumbral filaments
--Sunspot groups
---Bipolar sunspot groups
--Sunspot number
--Wilson effect
Solar system astronomy
-Earth-moon system
-Lunar science
--Lunar atmosphere
--Lunar evolution
--Lunar origin
--Lunar phase
--Lunar theory
---Annual equation
---Anomalistic month
---Lunar node regression
--Selenology
---Lunar features
----Lunar craters
----Lunar domes
----Lunar highlands
----Lunar maria
----Lunar mountains
----Lunar rays
----Lunar rilles
----Lunar transient phenomena
---Lunar geodesy
---Lunar gravitational field
---Lunar interior
----Lunar composition
----Lunar seismology
---Lunar magnetic fields
---Lunar surface
----Lunar geochronology
----Lunar impacts
----Lunar mineralogy
----Lunar petrology
-Planetary science
--Atmospheric science
---Aeronomy
---Atmospheric effects
----Seasonal phenomena
----Sky brightness
-----Night sky brightness
------Gegenschein
-----Twilight
--Impact phenomena
--Interplanetary magnetic fields
--Interplanetary physics
---Cometary studies
----Comet interiors
----Cometary atmospheres
----Cometary ionospheres
----Dirty snowball theory
---Corotating streams
---Interplanetary discontinuities
---Interplanetary particle acceleration
---Interplanetary shocks
---Interplanetary turbulence
---Meteor showers
----Meteor radiants
---Meteorite composition
---Pickup ions
---Planetary bow shocks
---Solar energetic particles
---Solar wind termination
--Planetary alignment
--Planetary atmospheres
---Atmospheric tides
---Earth atmosphere
----Atmospheric circulation
----Atmospheric tides
----Clouds
-----Cirrus castellanus
-----Cirrus fibratus
-----Cirrus floccus
-----Cirrus spissatus
-----Cirrus uncinus
-----Cirrus vertebratus
-----Noctilucent clouds
----Exosphere
-----Geocorona
----Greenhouse gases
-----Carbon dioxide
-----Chlorofluorocarbons
-----Methane
-----Nitrous oxide
-----Water vapor
----Humidity
----Ionosphere
-----D layer
-----E layer
-----F layer
----Land-atmosphere interactions
----Magnetosphere
-----Plasmapause
-----Van Allen radiation belt
----Mesosphere
----Ocean-atmosphere interactions
----Ozone layer
----Stratopause
----Stratosphere
----Thermosphere
----Tropopause
----Troposphere
---Planetary boundary layers
---Scale height
---Stratopause
---Upper atmosphere
---Water vapor
--Planetary structure
---Hydrosphere
---Lithosphere
---Mantle
---Oblateness
---Planetary cores
---Planetary interior
---Planetary polar regions
---Plate tectonics
---Polar caps
---Volcanoes
--Planetary system formation
---Planet formation
---Protoplanetary disks
----Planetesimals
---Solar system formation
--Planetary theory
--Satellite formation
--Solar-planetary interactions
---Solar-terrestrial interactions
--Surface gravity
-Solar system
--Asteroid belt
--Heliosphere
---Heliopause
---Heliosheath
---Stellar bow shocks
---Termination shock
--Interplanetary medium
---Interplanetary dust
----Meteoroid dust clouds
----Zodiacal cloud
---Interplanetary gas
---Interplanetary grains
---Protoplanetary disks
----Planetesimals
--Kuiper belt
---Trans-Neptunian objects
----Classical Kuiper belt objects
-----Borasisi
-----Chaos
-----Deucalion
-----Logos
-----Makemake
-----Quaoar
-----Teharonhiawako
-----Varuna
----Detached objects
----Neptune trojans
----Plutoids
-----Eris
-----Haumea
-----Makemake
-----Pluto
-----Quaoar
-----Sedna
----Resonant Kuiper belt objects
-----Plutinos
------Huya
------Ixion
------Orcus
------Pluto
-----Scattered disk objects
------Eris
------Sedna
-----Twotinos
--Meteoroids
---Meteorites
----Achondrites
----Aerolites
----Ataxites
----Bediasites
----Chondrites
-----Carbonaceous chondrites
-----Chondrules
----Iron meteorites
----Micrometeorites
----Moldavites
----Tektites
-----Australites
-----Bediasites
-----Indochinites
-----Moldavites
---Meteors
----Fireballs
-----Bolides
----Meteor streams
----Meteor trails
---Micrometeoroids
--Meteors
---Fireballs
----Bolides
---Meteor streams
---Meteor trails
--Natural satellites
---Jovian satellites
----Galilean satellites
---Martian satellites
---Neptunian satellites
---Saturnian satellites
---The Moon
---Uranian satellites
--Oort cloud
---Oort cloud objects
--Planetary rings
---Ansae
---Planetary ring divisions
---Shepherd satellites
---Spokes
--Planets [Solar system]
---Inner planets
----Earth (planet)
----Mars
----Mercury
----Venus
---Outer planets
----Jupiter
----Neptune
----Saturn
----Uranus
--Small solar system bodies
---Asteroids
----Hilda group
----Hirayama families
----Hungaria group
----Near-Earth objects
-----Amor group
-----Apollo group
-----Aten group
-----Atira group
-----Earth trojans
----Trojan asteroids
-----Earth trojans
-----Jupiter trojans
-----Mars trojans
-----Neptune trojans
---Comets
----Aperiodic comets
----Comas
----Comet tails
-----Comet tail streamers
----Kreutz Sungrazers
----Long period comets
-----Oort cloud
------Oort cloud objects
----Short period comets
---Minor planets
----Centaurs
----Dwarf planets
-----Ceres
-----Eris
-----Haumea
-----Makemake
-----Pluto
----Hilda group
----Hirayama families
----Hungaria group
----Trans-Neptunian objects
-----Classical Kuiper belt objects
------Borasisi
------Chaos
------Deucalion
------Logos
------Makemake
------Quaoar
------Teharonhiawako
------Varuna
-----Detached objects
-----Neptune trojans
-----Plutoids
------Eris
------Haumea
------Makemake
------Pluto
------Quaoar
------Sedna
-----Resonant Kuiper belt objects
------Plutinos
-------Huya
-------Ixion
-------Orcus
-------Pluto
------Scattered disk objects
-------Eris
-------Sedna
------Twotinos
--Solar neighborhood
--The Moon
--The Sun
Stellar astronomy
-Asteroseismology
--Oblique rotators
--Stellar magnetic fields
--Stellar oscillations
---Rapid stellar oscillations
---Solar oscillations
-Circumstellar matter
--Circumstellar clouds
--Circumstellar disks
---Debris disks
----Exozodiacal dust
----Planetesimals
---Protoplanetary disks
----Planetesimals
--Circumstellar dust
--Circumstellar envelopes
--Circumstellar gas
--Circumstellar grains
--Circumstellar masers
--Circumstellar shells
---Dust shells
---Rotating shells
---Shell burning
-Star clusters
--Globular star clusters
--Stellar associations
---Moving clusters
---O associations
---OB associations
---Open star clusters
----O clusters
----Young star clusters
---Protoclusters
---R associations
---T associations
-Stellar physics
--Star formation
---Star forming regions
--Starspots
--Stellar atmospheres
---Chromospheres
---Coronae
----Coronal dimming
----Coronal hole
----Coronal lines
----Coronal loops
----Coronal plumes
----Coronal transients
----E corona
----F corona
----K corona
----Solar corona
-----M region
-----Solar coronal holes
-----Solar coronal loops
-----Solar coronal streamers
-----Solar transition region
---Photospheres
----Granule
----Stellar faculae
--Stellar dynamics
---Supernova dynamics
--Stellar evolution
---Asymptotic giant branch
---Blue straggler stars
---Carbon flashes
---Early stellar evolution
---Eruptive phenomena
---Initial mass function
---Late stellar evolution
----Dredge-up
----Stellar accretion disks
---Nonstandard evolution
---Pre-main sequence evolution
----Helmholtz-Kelvin contraction
---Supernova evolution
---White dwarf evolution
--Stellar phenomena
---Astrosphere interstellar medium interactions
---Burst astrophysics
----Gamma-ray bursts
----Optical bursts
----Radio bursts
----Rapid bursts
----X-ray bursts
---Coronal mass ejections
---Stellar flares
----Disk flaring
----Optical flares
----Stellar x-ray flares
---Stellar mass loss
----Plasma jets
---Stellar pulsations
----Multi-periodic pulsation
-----Double-mode pulsation
----Non-radial pulsations
----Pulsation modes
----Radial pulsations
--Stellar processes
---Stellar diffusion
--Stellar properties
---Expanding stellar envelopes
---Starlight polarization
---Stellar abundances
----Beryllium abundance
----Boron abundance
----Helium abundance
----Lithium abundance
---Stellar accretion
---Stellar activity
---Stellar ages
---Stellar colors
---Stellar effective temperatures
---Stellar luminosities
---Stellar magnetic fields
---Stellar mass functions
---Stellar masses
---Stellar oscillations
----Rapid stellar oscillations
----Solar oscillations
---Stellar radii
---Stellar rotation
----Gravity darkening
----Radiative braking
---Stellar spectral lines
--Stellar structures
---Circumstellar shells
----Dust shells
----Rotating shells
----Shell burning
---Convective envelopes
----Convective shells
---Convective zones
---Polytropes
---Stellar composition
----Stellar chemical composition
----Stellar elemental abundances
---Stellar gas distribution
---Stellar interiors
----Stellar cores
-----Stellar inner cores
---Stellar surfaces
---Strömgren spheres
--Stellar winds
-Stellar populations
--Intermediate population stars
--Population I stars
--Population II stars
---Disk population
---Disk stars
---Horizontal branch stars
----Extreme horizontal branch stars
----Zero-age horizontal branch stars
---Population II Cepheid stars
---RR Lyrae variable stars
----Bailey type stars
----RRA stars
----RRab stars
----RRb stars
----RRc stars
---SX Phoenicis variable stars
--Population III stars
-Stellar remnants
--Compact objects
---Black holes
----Astrophysical black holes
-----Intermediate-mass black holes
-----Primordial black holes
-----Stellar mass black holes
-----Supermassive black holes
------Quasars
-------Broad-absorption line quasar
-------Double quasars
-------Individual quasars
-------Quasar-galaxy pairs
-------Radio loud quasars
-------Radio quiet quasars
-------X-ray quasars
----Classical black holes
-----Charged black holes
------Kerr-Newman black holes
------Reissner–Nordström black holes
-----Nonrotating black holes
------Reissner–Nordström black holes
------Schwarzschild black holes
-----Rotating black holes
------Kerr black holes
-------Maximal Kerr black holes
------Kerr-Newman black holes
-----Uncharged black holes
------Kerr black holes
-------Maximal Kerr black holes
------Schwarzschild black holes
---Compact binary systems
----Cataclysmic variable stars
-----AM Herculis stars
-----Nova-like variable stars
------AM Canum Venaticorum stars
------UX Ursae Majoris stars
------VY Sculpturis stars
-----Novae
------Classical novae
------Dwarf novae
-------SU Ursae Majoris stars
-------SX Arietis variable stars
-------U Geminorum stars
-------WZ Sagittae stars
-------Z Camelopardalis stars
------Fast novae
------Recurrent novae
------Slow novae
-------DQ Herculis stars
------Symbiotic novae
------X-ray novae
-----SX Arietis variable stars
-----Symbiotic novae
-----UV Persei stars
----Compact binary components
-----Black holes
------Astrophysical black holes
-------Intermediate-mass black holes
-------Primordial black holes
-------Stellar mass black holes
-------Supermassive black holes
--------Quasars
---------Broad-absorption line quasar
---------Double quasars
---------Individual quasars
---------Quasar-galaxy pairs
---------Radio loud quasars
---------Radio quiet quasars
---------X-ray quasars
------Classical black holes
-------Charged black holes
--------Kerr-Newman black holes
--------Reissner–Nordström black holes
-------Nonrotating black holes
--------Reissner–Nordström black holes
--------Schwarzschild black holes
-------Rotating black holes
--------Kerr black holes
---------Maximal Kerr black holes
--------Kerr-Newman black holes
-------Uncharged black holes
--------Kerr black holes
---------Maximal Kerr black holes
--------Schwarzschild black holes
-----Neutron stars
------Magnetars
-------Soft gamma ray repeaters
------Neutron star cores
------Pulsars
-------Binary pulsars
-------Millisecond pulsars
-------Optical pulsars
-------Radio pulsars
-------Rotation powered pulsars
------Relativistic stars
-------Relativistic binary stars
-----White dwarf stars
------DA stars
------DB stars
------DC stars
------DO stars
-------BL Herculis stars
-------PG 1159 stars
------DQ stars
------DZ stars
------ZZ Ceti stars
----Compact binary stars
-----Binary pulsars
-----X-ray binary stars
------High-mass X-ray binary stars
------Low-mass X-ray binary stars
-------Hz Herculis stars
------X-ray bursters
--Degenerate matter
--Ejecta
--Supernovae
---Core-collapse supernovae
----Type Ib supernovae
----Type Ic supernovae
----Type II supernovae
---Hypernovae
---Type Ia supernovae
-Stellar types
--Blue straggler stars
--Brown dwarf stars
---L dwarf stars
---L subdwarf stars
---T dwarf stars
---T subdwarf stars
---Y dwarf stars
--Chemically peculiar stars
---Am stars
---Ap stars
----Holmium stars
----Manganese stars
----Silicon stars
---Bp stars
---Carbon stars
----N stars
----R stars
---Heavy metal stars
----Barium stars
-----Semi-barium stars
----Manganese stars
----S stars
-----Zirconium stars
----Strontium stars
----Technetium stars
---Helium weak stars
---Helium-poor stars
----BW stars
---Helium-rich stars
----DB stars
---Hydrogen deficient stars
----AM Canum Venaticorum stars
---Lithium stars
---Magnetic stars
----Am stars
----Bp stars
----Magnetars
-----Soft gamma ray repeaters
----Magnetic variable stars
-----Alpha2 Canum Venaticorum stars
-----Am stars
-----SX Arietis variable stars
----Mercury-manganese stars
---Manganese stars
---Mercury-manganese stars
---Peculiar giants
---Peculiar variable stars
---Shell stars
---Strontium stars
---Technetium stars
---Zirconium stars
--Emission line stars
---Be type stars
---Early-type emission stars
----Ae stars
-----Herbig Ae/Be stars
----Be stars
-----Herbig Ae/Be stars
-----Lambda Eridani stars
----Oe stars
----Oef stars
----Of stars
----Wolf-Rayet stars
-----WC stars
-----WCN stars
-----WN stars
---Flash stars
---Gamma Cassiopeiae stars
---H-alpha stars
---Luminous blue variable stars
---Me stars
---Me variable stars
---Mira variable stars
---RC Aurigae stars
---S Doradus stars
---Symbiotic binary stars
----RR Telescopii stars
----Symbiotic novae
----Z Andromedae stars
---T Tauri stars
----Classical T Tauri stars
----FU Orionis stars
----Weak-line T Tauri stars
---X-ray stars
----Single X-ray stars
---Z Andromedae stars
--Evolved stars
---Giant stars
----A giant stars
----B giant stars
----CH stars
----CN stars
----Extreme carbon stars
----F giant stars
----G giant stars
----Late-type giant stars
-----Heavy metal stars
------Barium stars
-------Semi-barium stars
------Manganese stars
------S stars
-------Zirconium stars
------Strontium stars
------Technetium stars
-----Irregular variable stars
------Delta Scuti variable stars
------Gamma Cassiopeiae stars
------LC variable stars
------Mira variable stars
------R Coronae Borealis variable stars
------RC Aurigae stars
------Soft gamma ray repeaters
------T Tauri stars
-------Classical T Tauri stars
-------FU Orionis stars
-------Weak-line T Tauri stars
------UU Herculis stars
-----K giant stars
-----M giant stars
------Me variable stars
-----Mira variable stars
-----Semi-regular variable stars
------S Vulpeculae stars
----LB variable stars
----O giant stars
----OH/IR stars
----Peculiar giants
----R stars
----Red giant stars
-----Red straggler stars
----S stars
-----Zirconium stars
----Weak G band stars
---High-mass stars
----High-mass X-ray binary stars
---Hypergiant stars
----Yellow hypergiant stars
---Subgiant stars
----A subgiant stars
----B subgiant stars
----F subgiant stars
----G subgiant stars
----K subgiant stars
----M subgiant stars
----O subgiant stars
---Supergiant stars
--Main sequence stars
---Early-type stars
----A stars
-----A dwarf stars
-----A giant stars
-----A subdwarf stars
-----A subgiant stars
-----A supergiant stars
-----Ae stars
------Herbig Ae/Be stars
-----Am stars
-----Ap stars
------Holmium stars
------Manganese stars
------Silicon stars
----B stars
-----53 Persei stars
-----B dwarf stars
-----B giant stars
-----B subdwarf stars
-----B subgiant stars
-----B supergiant stars
-----Be stars
------Herbig Ae/Be stars
------Lambda Eridani stars
-----Bp stars
-----BW stars
-----Mercury-manganese stars
----Early-type emission stars
-----Ae stars
------Herbig Ae/Be stars
-----Be stars
------Herbig Ae/Be stars
------Lambda Eridani stars
-----Oe stars
-----Oef stars
-----Of stars
-----Wolf-Rayet stars
------WC stars
------WCN stars
------WN stars
----Early-type supergiant stars
-----A supergiant stars
-----B supergiant stars
-----O supergiant stars
-----OB supergiant stars
----Early-type supergiant stars
-----A supergiant stars
-----B supergiant stars
-----O supergiant stars
-----OB supergiant stars
----Early-type variable stars
-----Beta Cephei stars
-----Luminous blue variable stars
-----S Doradus stars
-----SX Arietis variable stars
----F supergiant stars
-----UU Herculis stars
----Faint blue stars
----G supergiant stars
----Late-type supergiant stars
-----K supergiant stars
-----M supergiant stars
----O stars
-----O dwarf stars
-----O giant stars
-----O subdwarf stars
-----O subgiant stars
-----O supergiant stars
-----Oe stars
-----Oef stars
-----Of stars
----OB stars
-----OB supergiant stars
----Red supergiant stars
---Intermediate type stars
----F stars
-----F dwarf stars
-----F giant stars
-----F subdwarf stars
-----F subgiant stars
-----F supergiant stars
------UU Herculis stars
----G stars
-----G dwarf stars
-----G giant stars
-----G subdwarf stars
-----G subgiant stars
-----G supergiant stars
---Late-type stars
----K stars
-----K dwarf stars
-----K giant stars
-----K subdwarf stars
-----K subgiant stars
-----K supergiant stars
----Late-type dwarf stars
-----K dwarf stars
-----L dwarf stars
-----M dwarf stars
-----T dwarf stars
----Late-type giant stars
-----Heavy metal stars
------Barium stars
-------Semi-barium stars
------Manganese stars
------S stars
-------Zirconium stars
------Strontium stars
------Technetium stars
-----Irregular variable stars
------Delta Scuti variable stars
------Gamma Cassiopeiae stars
------LC variable stars
------Mira variable stars
------R Coronae Borealis variable stars
------RC Aurigae stars
------Soft gamma ray repeaters
------T Tauri stars
-------Classical T Tauri stars
-------FU Orionis stars
-------Weak-line T Tauri stars
------UU Herculis stars
-----K giant stars
-----M giant stars
------Me variable stars
-----Mira variable stars
-----Semi-regular variable stars
------S Vulpeculae stars
----Late-type supergiant stars
-----K supergiant stars
-----M supergiant stars
----M stars
-----M dwarf stars
-----M giant stars
------Me variable stars
-----M subdwarf stars
-----M subgiant stars
-----M supergiant stars
-----Me stars
----N stars
----R stars
----S stars
-----Zirconium stars
---Yellow stragglers
---Zero-age main sequence stars
--Multiple stars
---Binary stars
----Astrometric binary stars
----Close binary stars
-----Accreting binary stars
-----Algol variable stars
-----Compact binary stars
-----Contact binary stars
------Binary pulsars
------X-ray binary stars
-------High-mass X-ray binary stars
-------Low-mass X-ray binary stars
--------Hz Herculis stars
-------X-ray bursters
-----Ellipsoidal variable stars
------Beta Lyrae stars
-----Eruptive binary stars
------Dwarf novae
-------SU Ursae Majoris stars
-------SX Arietis variable stars
-------U Geminorum stars
-------WZ Sagittae stars
-------Z Camelopardalis stars
------Symbiotic binary stars
-------RR Telescopii stars
-------Symbiotic novae
-------Z Andromedae stars
------X-ray binary stars
-------High-mass X-ray binary stars
-------Low-mass X-ray binary stars
--------Hz Herculis stars
-------X-ray bursters
-----Interacting binary stars
------Cataclysmic variable stars
-------AM Herculis stars
-------Nova-like variable stars
--------AM Canum Venaticorum stars
--------UX Ursae Majoris stars
--------VY Sculpturis stars
-------Novae
--------Classical novae
--------Dwarf novae
---------SU Ursae Majoris stars
---------SX Arietis variable stars
---------U Geminorum stars
---------WZ Sagittae stars
---------Z Camelopardalis stars
--------Fast novae
--------Recurrent novae
--------Slow novae
---------DQ Herculis stars
--------Symbiotic novae
--------X-ray novae
-------SX Arietis variable stars
-------Symbiotic novae
-------UV Persei stars
------X-ray binary stars
-------High-mass X-ray binary stars
-------Low-mass X-ray binary stars
--------Hz Herculis stars
-------X-ray bursters
-----Semi-detached binary stars
-----Z Andromedae stars
----Companion stars
-----Substellar companion stars
-----Tertiary stars
----Detached binary stars
----Eclipsing binary stars
-----Algol variable stars
-----Beta Lyrae stars
-----Upsilon Sagittarii stars
----Interferometric binary stars
----Relativistic binary stars
----Semi-detached binary stars
----Spectroscopic binary stars
-----Two-spectrum binary stars
----Visual binary stars
----Wide binary stars
---Trinary stars
--Novae
---Classical novae
---Dwarf novae
----SU Ursae Majoris stars
----SX Arietis variable stars
----U Geminorum stars
----WZ Sagittae stars
----Z Camelopardalis stars
---Fast novae
---Recurrent novae
---Slow novae
----DQ Herculis stars
---Symbiotic novae
---X-ray novae
--Protostars
---Bok globules
---Cocoon stars
---Cometary nebulae
---Proplyds
---Young stellar objects
----Pre-main sequence stars
-----Herbig Ae/Be stars
-----Herbig-Haro objects
-----T Tauri stars
------Classical T Tauri stars
------FU Orionis stars
------Weak-line T Tauri stars
--Supernovae
---Core-collapse supernovae
----Type Ib supernovae
----Type Ic supernovae
----Type II supernovae
---Hypernovae
---Type Ia supernovae
--Variable stars
---Extrinsic variable stars
----Eclipsing binary stars
-----Algol variable stars
-----Beta Lyrae stars
-----Upsilon Sagittarii stars
----Ellipsoidal variable stars
-----Beta Lyrae stars
---Intrinsic variable stars
----Cataclysmic variable stars
-----AM Herculis stars
-----Nova-like variable stars
------AM Canum Venaticorum stars
------UX Ursae Majoris stars
------VY Sculpturis stars
-----Novae
------Classical novae
------Dwarf novae
-------SU Ursae Majoris stars
-------SX Arietis variable stars
-------U Geminorum stars
-------WZ Sagittae stars
-------Z Camelopardalis stars
------Fast novae
------Recurrent novae
------Slow novae
-------DQ Herculis stars
------Symbiotic novae
------X-ray novae
-----SX Arietis variable stars
-----Symbiotic novae
-----UV Persei stars
----Eruptive variable stars
-----Flare stars
------BY Draconis stars
------FU Orionis stars
------R Coronae Borealis variable stars
------Red dwarf flare stars
------RS Canum Venaticorum variable stars
------UV Ceti stars
----Herbig-Haro objects
----Long period variable stars
-----Mira variable stars
-----Semi-regular variable stars
------S Vulpeculae stars
-----Slow irregular variable stars
-----WZ Sagittae stars
----Magnetic variable stars
-----Alpha2 Canum Venaticorum stars
-----Am stars
-----SX Arietis variable stars
----Pulsating variable stars
-----53 Persei stars
-----Beta Cephei stars
-----Cepheid variable stars
------Delta cephei
------Double-mode Cepheid variable stars
------W Virginis variable stars
-------BL Herculis stars
------Young disk Cepheid variable stars
-----Delta Delphini stars
-----Delta Scuti variable stars
-----Double-mode variable stars
------Double-mode Cepheid variable stars
------RR Lyrae variable stars
-------Bailey type stars
-------RRA stars
-------RRab stars
-------RRb stars
-------RRc stars
-----Irregular variable stars
------Delta Scuti variable stars
------Gamma Cassiopeiae stars
------LC variable stars
------Mira variable stars
------R Coronae Borealis variable stars
------RC Aurigae stars
------Soft gamma ray repeaters
------T Tauri stars
-------Classical T Tauri stars
-------FU Orionis stars
-------Weak-line T Tauri stars
------UU Herculis stars
-----Lambda Eridani stars
-----Long period variable stars
------Mira variable stars
------Semi-regular variable stars
-------S Vulpeculae stars
------Slow irregular variable stars
------WZ Sagittae stars
-----Mira variable stars
-----Multi-periodic variable stars
------Beta Cephei stars
------Delta Scuti variable stars
------Double-mode variable stars
-------Double-mode Cepheid variable stars
-------RR Lyrae variable stars
--------Bailey type stars
--------RRA stars
--------RRab stars
--------RRb stars
--------RRc stars
------PG 1159 stars
------SX Phoenicis variable stars
------ZZ Ceti stars
-----PV Telescopii variable stars
-----RV Tauri variable stars
-----S Vulpeculae stars
-----Semi-regular variable stars
------S Vulpeculae stars
---Periodic variable stars
----Long period variable stars
-----Mira variable stars
-----Semi-regular variable stars
------S Vulpeculae stars
-----Slow irregular variable stars
-----WZ Sagittae stars
----Multi-periodic variable stars
-----Beta Cephei stars
-----Delta Scuti variable stars
-----Double-mode variable stars
------Double-mode Cepheid variable stars
------RR Lyrae variable stars
-------Bailey type stars
-------RRA stars
-------RRab stars
-------RRb stars
-------RRc stars
-----PG 1159 stars
-----SX Phoenicis variable stars
-----ZZ Ceti stars
----Semi-regular variable stars
-----S Vulpeculae stars
----Short period variable stars
-----Beta Cephei stars
-----Delta Scuti variable stars
--White dwarf stars
---DA stars
---DB stars
---DC stars
---DO stars
----BL Herculis stars
----PG 1159 stars
---DQ stars
---DZ stars
---ZZ Ceti stars
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Caitlin Casey con Helmut Dannerbauer durante su estancia en el IAC
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ESPRESSO
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The mayor of Güímar visits the Teide Observatory
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Visita del embajador de Japón
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Visita de la Corporación Municipal de Tegueste
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I Jornada sobre sobre Protección del Cielo y Oportunidades de Empleo
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Presentación del libro “Observando el Sol desde Tenerife” de Manuel Vázquez Abeledo
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Presentación del informe sobre impacto socio-económico del TMT en La Palma
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Calendario astronómico 2020
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Semanas de la Ciencia 2019
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Future Instruments for the Telescopes at the Observatorios de Canarias
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ESFRI en La Palma
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Visita del Cónsul de Japón en Canarias
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DESI
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HC2NP2019
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Amanar: bajo el mismo cielo
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