| Publicación |
The star formation history and dust content in the far outer disc of M31 |
iacweb |
Hace 2 months 1 week |
| Publicación |
The Carina Project. V. The Impact of NLTE Effects on the Iron Content |
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The Sloan Digital Sky Survey quasar catalog: ninth data release |
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A Three-dimensional View of the Remnant of Nova Persei 1901 (GK Per) |
iacweb |
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The Nature of Dust in Compact Galactic Planetary Nebulae from Spitzer Spectra |
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IPHAS and the symbiotic stars . II. New discoveries and a sample of the most common mimics |
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Angular Size Test on the Expansion of the Universe |
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47 new T dwarfs from the UKIDSS Large Area Survey |
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Blue not brown: UKIRT Infrared Deep Sky Survey T dwarfs with suppressed K-band flux |
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The discovery of the T8.5 dwarf UGPS J0521+3640 |
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Disc frequencies for brown dwarfs in the Upper Scorpius OB association: implications for brown dwarf formation theories |
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Discovery of the benchmark metal-poor T8 dwarf BD +01° 2920B |
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The Return of the Bursts: Thermonuclear Flashes from Circinus X-1 |
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The activity of comet C/2007 D1 (LINEAR) at 9.7 AU from the Sun |
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Rotational fission of trans-Neptunian objects: the case of Haumea |
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Cosmic rays linked to rapid mid-latitude cloud changes |
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Spectroscopic characterization of a sample of metal-poor solar-type stars from the HARPS planet search program. Precise spectroscopic parameters and mass estimation |
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Fluorine abundances in dwarf stars of the solar neighbourhood |
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Low Mg/Si Planetary Host Stars and Their Mg-depleted Terrestrial Planets |
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Chemical abundances of 1111 FGK stars from the HARPS GTO planet search program. Galactic stellar populations and planets |
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Infrared spectroscopy of hydrogenated fullerenes (fulleranes) at extreme temperatures |
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The supergiant optical counterpart of ULX P13 in NGC 7793 |
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The Nature of the UV/Optical Emission of the Ultraluminous X-Ray Source in Holmberg II |
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The young stellar population of IC 1613. II. Physical properties of OB associations |
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The IACOB project: A grid-based automatic tool for the quantitative spectroscopic analysis of O-stars |
iacweb |
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