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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  • Water ice and organics on the surface of the asteroid 24 Themis
    It has been suggested that Earth's current supply of water was delivered by asteroids, some time after the collision that produced the Moon (which would have vaporized any of the pre-existing water). So far, no measurements of water ice on asteroids have been made, but its presence has been inferred from the comet-like activity of several small
    Campins, Humberto et al.

    Fecha de publicación:

    4
    2010
    Número de citas
    271
  • Variability in Nearby Ultracool Dwarfs
    Variability is a key property of ultracool dwarfs as it may induce physical noise that limits the accuracy of radial velocities. In this paper we report on our current activities in the study of variability in ultracool dwarfs.
    Martin, E. L. et al.

    Fecha de publicación:

    4
    2010
    Número de citas
    0
  • Underground seeing: characterization of geological hazard at the astronomical observatories of the Canaries, Chile and Hawaii
    Not Available
    Eff-Darwich, A.

    Fecha de publicación:

    4
    2010
    Número de citas
    0
  • UBVRI photometry in Be 15, Be 80 and NGC 2192 (Tapia+, 2010)
    The CCD UBV(RI)C observations of this paper have been made exclusively with the 0.84-m f/15 Ritchey-Chretien telescope at SPM, during the night of 2001 June 25/26 for the open cluster Be 80, and the nights 2002 February 6/7 and 8/9 for the clusters NGC 2192 and Be 15, respectively. (3 data files).
    Tapia, M. T. et al.

    Fecha de publicación:

    4
    2010
    Número de citas
    0
  • Three-dimensional Propagation of Magnetohydrodynamic Waves in Solar Coronal Arcades
    We numerically investigate the excitation and temporal evolution of oscillations in a two-dimensional coronal arcade by including the three-dimensional propagation of perturbations. The time evolution of impulsively generated perturbations is studied by solving the linear, ideal magnetohydrodynamic (MHD) equations in the zero-β approximation. As we
    Rial, S. et al.

    Fecha de publicación:

    4
    2010
    Número de citas
    7