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Multi-fibre optical spectroscopy of low-mass stars and brown dwarfs in Upper Scorpius |
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What ignites on the neutron star of 4U 0614+091? |
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The double-peaked 2008 outburst of the accreting milli-second X-ray pulsar, IGR J00291+5934 |
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Type I X-ray bursts and burst oscillations in the accreting millisecond X-ray pulsar IGR J17511-3057 |
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Discovery of an Accreting Millisecond Pulsar in the Eclipsing Binary System SWIFT J1749.4-2807 |
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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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New observations of asteroid (175706) 1996 FG3, primary target of the ESA Marco Polo-R mission |
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EPOXI: Comet 103P/Hartley 2 Observations from a Worldwide Campaign |
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The spectrum of (136199) Eris between 350 and 2350 nm: results with X-Shooter |
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Links between the dynamical evolution and the surface color of the Centaurs |
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Near-infrared spectroscopic survey of B-type asteroids: Compositional analysis |
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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. II. Doppler velocities<xref ref-type="fn" rid="FN1"> |
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The James Clerk Maxwell Telescope Nearby Galaxies Legacy Survey. II. Warm Molecular Gas and Star Formation in Three Field Spiral Galaxies |
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Photometric scaling relations of lenticular and spiral galaxies |
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Near-infrared atlas of S0-Sa galaxies (NIRS0S) |
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European Extremely Large Telescope Site Characterization I: Overview |
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Morphological Parameters of a Spitzer Survey of Stellar Structure in Galaxies |
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Amino acids in comets and meteorites: stability under gamma radiation and preservation of the enantiomeric excess |
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Infrared spectroscopy and integrated molar absorptivity of C60 and C70 fullerenes at extreme temperatures |
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Doppler imaging of the double-lined active binary V824 Ara |
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Analysis of chemical abundances in planetary nebulae with [WC] central stars. I. Line intensities and physical conditions |
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Planck intermediate results. XIII. Constraints on peculiar velocities |
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Constraining clumpy dusty torus models using optimized filter sets |
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