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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  • A candidate super-Earth planet orbiting near the snow line of Barnard's star
    Barnard's star is a red dwarf, and has the largest proper motion (apparent motion across the sky) of all known stars. At a distance of 1.8 parsecs1, it is the closest single star to the Sun; only the three stars in the α Centauri system are closer. Barnard's star is also among the least magnetically active red dwarfs known2,3 and has an estimated
    Ribas, I. et al.

    Fecha de publicación:

    11
    2018
    Número de citas
    121
  • A catalogue of the observations of the mutual phenomena of the Galilean satellites made in 1991 during the PHEMU91 campaign
    In this paper, all the light-curves obtained during the PHEMU91 campaign of observations of the mutual phenomena of the Galilean satellites are presented. These observations give accurate astrometric positions of major interest for dynamical studies of the motion of the Galilean satellites. The aim of this work is to give observational data
    Arlot, J. E. et al.

    Fecha de publicación:

    11
    1997
    Número de citas
    22
  • A chemical survey of exoplanets with ARIEL
    Thousands of exoplanets have now been discovered with a huge range of masses, sizes and orbits: from rocky Earth-like planets to large gas giants grazing the surface of their host star. However, the essential nature of these exoplanets remains largely mysterious: there is no known, discernible pattern linking the presence, size, or orbital
    Tinetti, Giovanna et al.

    Fecha de publicación:

    11
    2018
    Número de citas
    282
  • A Companion Nuclear Bulge to the Seyfert Ring Galaxy NGC 985
    Subarcsecond optical broad band images of the Seyfert galaxy NGC 985 are presented. A second nucleus located 3.8" NW of the Seyfert nucleus is clearly revealed by these images and confirmed by the study of its colors and brightness profile. We claim that this object is a spheroidal bulge with an absolute magnitude M_B_ = -16.6, and that it is
    Perez Garcia, A. M. et al.

    Fecha de publicación:

    11
    1996
    Número de citas
    8
  • A composite H ii region luminosity function in Hα of unprecedented statistical weight
    Context: .Statistical properties of H ii region populations in disk galaxies yield important clues to the physics of massive star formation. Aims: .We present a set of H ii region catalogues and luminosity functions for a sample of 56 spiral galaxies in order to derive the most general form of their luminosity function. Methods: .H ii region
    Bradley, T. R. et al.

    Fecha de publicación:

    11
    2006
    Número de citas
    50
  • A consideration of the solar cycle in the light of the behavior of the large active regions
    The solar cycle was studied by considering only the large active regions (AR), with small region data being ignored. Results show that at birth almost all the large AR display the correct inclination (p-part at lower latitude) while the small AR show random behavior. The maximum latitude attained by the large AR is lower by 10 deg than that of the
    Garcia de la Rosa, J. I.

    Fecha de publicación:

    11
    1984
    Número de citas
    0