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A frequency comb calibrated solar atlas |
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Towards a dynamical mass of the ultraluminous X-ray source NGC 5408 X-1 |
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Discovery of a planetary nebula surrounding the symbiotic star DT Serpentis |
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Thermodynamic fluctuations in solar photospheric three-dimensional convection simulations and observations |
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Multiple stellar populations in Magellanic Cloud clusters. II. Evidence also in the young NGC 1844? |
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The first spectroscopically identified L dwarf in Praesepe |
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Kinematics of Arp 270: gas flows, nuclear activity and two regimes of star formation |
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Theoretical formulation of Doppler redistribution in scattering polarization within the framework of the velocity-space density matrix formalism |
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Stellar activity as a tracer of moving groups |
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On the Effects of the Evolution of Microbial Mats and Land Plants on the Earth as a Planet. Photometric and Spectroscopic Light Curves of Paleo-Earths |
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The Hanle Effect of Lyα in a Magnetohydrodynamic Model of the Solar Transition Region |
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Structure of Abell 1995 from optical and X-ray data: a galaxy cluster with an elongated radio halo |
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Excitation of emission lines by fluorescence and recombination in IC 418 |
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The shapes of BCGs and normal ellipticals in nearby clusters |
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Planck pre-launch status: Calibration of the Low Frequency Instrument flight model radiometers |
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Hace 10 months 1 week |
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H-ATLAS: PACS imaging for the Science Demonstration Phase |
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Hace 10 months 1 week |
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Numerical simulations of conversion to Alfvén waves in solar active regions |
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Spitzer Imaging of Herschel-atlas Gravitationally Lensed Submillimeter Sources |
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Hace 10 months 1 week |
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The spectral type of CHS 7797 - an intriguing very low mass periodic variable in the Orion Nebula Cluster |
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Hace 10 months 1 week |
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The second release of the Toruń catalogue of Galactic post-AGB objects: New classification scheme |
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VLT diffraction-limited imaging at 11 and 18μm of the nearest active galactic nuclei |
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The scaling of X-ray variability with luminosity in ultra-luminous X-ray sources |
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New groups of planetary nebulae with peculiar dust chemistry towards the Galactic bulge |
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Heavy Element Nucleosynthesis in the Brightest Galactic Asymptotic Giant Branch Stars |
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Prominence Thread Seismology Using the P 1/2P 2 Ratio |
iacweb |
Hace 10 months 1 week |