Tipo de publicación: Sin árbitro

  • Publicación
    Classification and vsini of Vega-type and PMS stars (Mora+, 2001)
    File table1.dat contains the log of the spectroscopic observations of the stars in the EXPORT sample taken with the Isaac Newton Telescope during the 1998...
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    Classification of Galaxies by Their Radial Profiles: Unbarred Early Types
    We classify 46 broad band surface-brightness profiles in the visible from a sample of nearby early-type unbarred galaxies imaged at the ING (La Palma) and in...
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    Classifying MaNGA galaxies with unsupervised machine learning techniques
    We explore the use of unsupervised machine learning to classify a sample of >9000 nearby galaxies of all types from the SDSS MaNGA survey. Our aim is to find a...
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    Climate diagnostic archives: an approach to ELT site selection
    Climate diagnostic studies combine data from different sources (radiosoundes, satellites, meteorological masts, etc) and meteorological models to predict the...
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    Climate Variability in the Levant basin during the last deglaciation
    Climate variability of the eastern part of the Mediterranean Sea during the last deglaciation has been reconstructed from a marine sediment core MD04-2722 (33...
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    Climatological databases as a tool for the ELT site selection
    Climate diagnostic archives appears to be a very useful tool for astronomical site assessment. These climatological databases combine data from meteorological...
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    Climatology at the Roque de LOS Muchachos Observatory
    The Roque de los Muchachos Observatory (ORM) at La Palma (Canary Islands) is one of the two top pre-selected sites for hosting the future European Extremely...
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    Close binaries and common envelopes
    David Jones, Jorge García-Rojas, Ondřej Pejcha and Roger Wesson report on their RAS Specialist Discussion Meeting exploring "Common envelope evolution and post...
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    Close binary central stars and the abundance discrepancy - new extreme objects
    Recent work (Corradi et al. 2015; Jones et al. 2016) has shown that the phenomenon of extreme abundance discrepancies, where recombination line abundances...