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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  • The starburst galaxy NGC 7714
    Narowband H alpha imaging and long-slit optical and near-infrared spectroscopy are analyzed in a study of the starburst galaxy NGC 7714. The data indicate that the galaxy as a whole is experiencing intense star formation activity; this is more conspicuous in the nucleus, where the star formation rate and the star formation rate per unit area are
    Gonzalez-Delgado, Rosa M. et al.

    Fecha de publicación:

    2
    1995
    Número de citas
    98
  • Supernova 1995D in NGC 2962
    IAUC 6135 available at Central Bureau for Astronomical Telegrams.
    Benetti, S. et al.

    Fecha de publicación:

    2
    1995
    Número de citas
    3
  • Structure and Evolution of Circumstellar Shells Formed by Massive Star Winds
    We follow the interaction of massive stars with their circumstellar gas over their entire life-times by combining hydrodynamic stellar evolution calculations for 35 and 60M &sun; stars and one- and two-dimensional gas dynamical calculations for the circumstellar medium.
    García-Segura, Guillermo et al.

    Fecha de publicación:

    2
    1995
    Número de citas
    0
  • SN 1991F in NGC 3458: A peculiar type IA supernova?
    Supernova 1991F appeared in the lenticular galaxy NGC 3458 (UGC 6037). On discovery, it was classified as type I, although no subtype (i.e., Ia or Ib/c) was assigned to it. In this paper, we present several low resolution spectra of this supernova. One of them was recorded ten days after the discovery. Two others show the supernova spectral
    Gomez, G. et al.

    Fecha de publicación:

    2
    1995
    Número de citas
    9
  • On the evolutionary status of two very active visual binaries
    HD 36705 (AB Doradus) and HD 155555 (V824 Ara) are two nearby very active cool stars. Both have strong Li I (lambda)6708 resonance lines, implying high surface Li abundances, comparable to those of very young T Tauri stars. They also have late M-type visual companions which share their proper motion, as confirmed by new astrometric measurements
    Brandner, Wolfgang et al.

    Fecha de publicación:

    2
    1995
    Número de citas
    31
  • LTE polarized radiative transfer through interlaced atmospheres
    We show that the solution of the radiative transfer equation (RTE) through a line of sight that pierces several times two alternate atmospheres can be obtained in terms of the solutions of the RTE through both single atmospheres separately considered. This also applies to the response functions of the observed Stokes spectrum to perturbations of
    del Toro Iniesta, J. C. et al.

    Fecha de publicación:

    2
    1995
    Número de citas
    5