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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  • Book Review: New windows to the universe (2 V.) / Cambridge U Press, 1990
    Not Available
    De Greve, J. P.

    Fecha de publicación:

    9
    1992
    Número de citas
    0
  • Bidimensional spectroscopy of the central kiloparsec of NGC 4151
    Sixty-one bidimensionally distributed spectra covering the circumnuclear region of NGC 4161 within a radius of about 6.5 arcsec are presented. The local conditions and the mean velocity field are studied from an analysis of the H-alpha, forbidden N II 6548, 6584, and forbidden S II 6716, 6731 lines. The alignment of the line intensity maps in the
    Mediavilla, E. et al.

    Fecha de publicación:

    9
    1992
    Número de citas
    24
  • "Remote" science with the NTT from Italy. Preliminary scientific results.
    Not Available
    Franchini, M. et al.

    Fecha de publicación:

    9
    1992
    Número de citas
    0
  • V1727 Cygni = 4U 2129+47
    IAUC 5578 available at Central Bureau for Astronomical Telegrams. IAUC 5578 available at Central Bureau for Astronomical Telegrams.
    Garcia, M. et al.

    Fecha de publicación:

    8
    1992
    Número de citas
    3
  • Stray-light effects on the solar intensity distribution
    A description of the stray-light problem based on a radiative transfer approach is presented. The 2D convolution that describes the effect of the stray-light is recovered in this formalism. The controversy raised by the old normalization condition is satisfactorily eliminated within the present description. The present formalism is applied to
    Martinez Pillet, V.

    Fecha de publicación:

    8
    1992
    Número de citas
    43
  • Observation of fine structure in the cold phase of the local interstellar medium using K I absorption
    The K I 7699-A resonance absorption line was used to observe a group of 18 early-type stars within a 200-pc radius of the sun with a signal-to-noise ratio of 50-250. The interstellar absorptions provide a way to 'tag' a cloud via its radial velocity to within +/-1.5 km/s. Based on the hypothesis of pressure confinement, the temperatures of the
    Trapero, Joaquin et al.

    Fecha de publicación:

    8
    1992
    Número de citas
    17