Tipo de publicación: Sin árbitro

  • Publicación
    A major step in understanding the X-ray generation in comets: recent progress obtained with XMM-Newton
    The observation of comet C/2000 WM1 (LINEAR) with XMM-Newton is a highlight in the field of cometary research. During 17 hours of almost uninterrupted...
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    A map-making algorithm for the QUIJOTE CMB experiment
    In the last years we obtained a very detailed picture of the Primordial Universe by, among other means, measuring the intensity and the polarization of the...
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    A mask quality control tool for the OSIRIS multi-object spectrograph
    OSIRIS multi object spectrograph uses a set of user-customised-masks, which are manufactured on-demand. The manufacturing process consists of drilling the...
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    A Massive AGB Star as Source of Short-Lived Nuclei in the Early Solar System
    The origin of short-lived radioactive nuclei at the time of the formation of the Sun is a much debated mystery in modern astronomy. We show that abundance...
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    A massive star odyssey : from main sequence to supernova : proceedings of the 212th Symposium of the International Astronomical Union held in Costa Teguise, Lanzarote, Canary Islands, 24-28 June 2002
    Not Available
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    A Method for an Accurate Simulation of Crowding Effects in Synthetic CM Diagrams
    Not Available
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    A Method for Calibrating, in Absolute Flux Units, CA II H Profiles of Late Type Stars Observed at ESO
    The authors have applied to the Sun a method for calibrating, in absolute flux units, Ca II H profiles of late-type stars. After comparing, in the region 3948 -...
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    A Method for Correcting Star Counts in Moderately Overcrowded Fields
    Not Available
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    A method of determining the inclination angle in cataclysmic variables
    Not Available