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Detection of Peptidic Sequences in the Ancient Acidic Sediments of Río Tinto, Spain |
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The Wendelstein Calar Alto Pixellensing Project (WeCAPP): the M 31 nova catalogue |
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First results from the POMME survey of M31 |
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Spider. IV. Optical and Near-infrared Color Gradients in Early-type Galaxies: New Insight into Correlations with Galaxy Properties |
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Far-infrared properties of submillimeter and optically faint radio galaxies |
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A first catalogue of automatically selected ultraviolet-excess sources from the UVEX survey |
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Scattering Polarization of Hydrogen Lines in Weakly Magnetized Stellar Atmospheres. I. Formulation and Application to Isothermal Models |
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MAGIC observation of the GRB 080430 afterglow |
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An eclipsing post-common-envelope binary in the field of the Kepler mission |
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Clear detection of dusty torus signatures in a weak-line radio galaxy: the case of PKS 0043-42 |
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Seismology of Standing Kink Oscillations of Solar Prominence Fine Structures |
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SDSS J163030.58+423305.8: a 40-min orbital period detached white dwarf binary |
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Evolution of blue E/S0 galaxies from z ~ 1: merger remnants or disk-rebuilding galaxies? |
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The most recent burst of star formation in the massive elliptical galaxy NGC 1052 |
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A Peculiar Young Eruptive Star in the Dark Cloud Lynds 1340 |
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New Times of Minima of Eclipsing Binary Systems |
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On the importance of the few most massive stars: The ionizing cluster of NGC 588 |
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Kinematic Modelling of the Sculptor Dwarf Spheroidal Galaxy |
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The Metallicity of Pregalactic Globular Clusters: The Observational Consequences of the First Stars |
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Kinematics of globular cluster systems and the formation of early-type galaxies |
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Performance of satellite-to-ground communications link between ARTEMIS and the Optical Ground Station |
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Observation of enhanced X-ray emission from the CTTS AA Tauri during one transit of an accretion funnel flow |
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Helioseismology program for the PICARD satellite |
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The Fundamental Plane for early-type galaxies: dependence on the magnitude range |
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Discovery of Two Very Low Mass Binaries: Final Results of an Adaptive Optics Survey of Nearby M6.0-M7.5 Stars |
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Hace 10 months 1 week |