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New Candidate Planetary Nebulae in the IPHAS Survey: the Case of Planetary Nebulae with ISM interaction |
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Hace 3 weeks 2 days |
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The new carbon symbiotic star IPHAS J205836.43+503307.2 |
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VISTA Variables in the Via Lactea (VVV): The public ESO near-IR variability survey of the Milky Way |
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VVV DR1: The first data release of the Milky Way bulge and southern plane from the near-infrared ESO public survey VISTA variables in the Vía Láctea |
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ɛ Indi Ba, Bb: a detailed study of the nearest known brown dwarfs |
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Discovery of a 205.89 Hz Accreting Millisecond X-ray Pulsar in the Globular Cluster NGC 6440 |
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The double-peaked 2008 outburst of the accreting milli-second X-ray pulsar, IGR J00291+5934 |
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The Return of the Bursts: Thermonuclear Flashes from Circinus X-1 |
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Investigating the disc-jet coupling in accreting compact objects using the black hole candidate Swift J1753.5-0127 |
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Discovery of an Accreting Millisecond Pulsar in the Eclipsing Binary System SWIFT J1749.4-2807 |
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On the Cooling Tails of Thermonuclear X-ray Bursts: The IGR J17480-2446 Link |
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The Faint "Heartbeats" of IGR J17091-3624: An Exceptional Black Hole Candidate |
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Millihertz Quasi-periodic Oscillations and Thermonuclear Bursts from Terzan 5: A Showcase of Burning Regimes |
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Water ice and organics on the surface of the asteroid 24 Themis |
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Observations, compositional, and physical characterization of near-Earth and Mars-crosser asteroids from a spectroscopic survey |
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The Origin of Asteroid 101955 (1999 RQ36) |
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(65) Cybele: detection of small silicate grains, water-ice, and organics |
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Stardust-NExT, Deep Impact, and the accelerating spin of 9P/Tempel 1 |
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EPOXI: Comet 103P/Hartley 2 Observations from a Worldwide Campaign |
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Near-infrared spectroscopy of primitive asteroid families |
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EURONEAR—Recovery, follow-up and discovery of NEAs and MBAs using large field 1-2 m telescopes |
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Links between the dynamical evolution and the surface color of the Centaurs |
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MarcoPolo-R near earth asteroid sample return mission |
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An active region filament studied simultaneously in the chromosphere and photosphere. I. Magnetic structure |
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An active region filament studied simultaneously in the chromosphere and photosphere. II. Doppler velocities<xref ref-type="fn" rid="FN1"> |
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Hace 3 weeks 2 days |