Publicaciones

Esta sección ofrece el acceso a la base de datos de Publicaciones que recopila los artículos del IAC publicados en revistas científicas. Por favor, pulsa la flecha del menú para ver todas las opciones de búsqueda y de ordenación de resultados; autor, revista, año, etc..

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  • Center-to-limb variation of the area covered by magnetic bright points in the quiet Sun
    Context. The quiet Sun magnetic fields produce ubiquitous bright points (BPs) that cover a significant fraction of the solar surface. Their contribution to the total solar irradiance (TSI) is so-far unknown. Aims: We aim at measuring the center-to-limb variation (CLV) of the fraction of solar surface covered by quiet Sun magnetic bright points. The
    Bonet, J. A. et al.

    Fecha de publicación:

    3
    2012
    Número de citas
    15
  • Biosignatures as revealed by spectropolarimetry of Earthshine
    Low-resolution intensity spectra of Earth's atmosphere obtained from space reveal strong signatures of life (`biosignatures'), such as molecular oxygen and methane with abundances far from chemical equilibrium, as well as the presence of a `red edge' (a sharp increase of albedo for wavelengths longer than 700nm) caused by surface vegetation. Light
    Sterzik, Michael F. et al.

    Fecha de publicación:

    3
    2012
    Número de citas
    91
  • Asteroseismology of the Solar Analogs 16 Cyg A and B from Kepler Observations
    The evolved solar-type stars 16 Cyg A and B have long been studied as solar analogs, yielding a glimpse into the future of our own Sun. The orbital period of the binary system is too long to provide meaningful dynamical constraints on the stellar properties, but asteroseismology can help because the stars are among the brightest in the Kepler field
    Metcalfe, T. S. et al.

    Fecha de publicación:

    3
    2012
    Número de citas
    160
  • ASK spectroscopic sequence of galaxies (Ascasibar+, 2011)
    We identify a spectroscopic sequence of galaxies, analogous to the Hubble sequence of morphological types, based on the Automatic Spectroscopic K-means-based (ASK) classification. Considering galaxy spectra as multidimensional vectors, the majority of the spectral classes are distributed along a well-defined curve going from the earliest to the
    Ascasibar, Y. et al.

    Fecha de publicación:

    3
    2012
    Número de citas
    0