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..

Además ofrece acceso al  repositorio de preprints del IAC: https://research.iac.es/preprints/l

  • Sin árbitro
    UV Spectroscopy of SN 1993J and Detection of Stellar Wind Material from the Progenitor
    Low and high resolution IUE spectra (1150-3200 Angstroms) of SN 1993J in NGC 3031 were obtained starting on 1993 March 30.2 UT. The initially strong ultraviolet continuum faded rapidly by April 4 (a factor of 200 at lambda
    Sonneborn, G. et al.

    Fecha de publicación:

    5
    1993
    Bibcode
    1993AAS...182.5503S
    Número de citas
    1
  • Con árbitro
    The optical properties of low luminosity radio galaxies with radio jets
    A morphological description and CCD photometric information for a sample of 24 low luminosity radio galaxies with radio jets are presented. It is concluded that Fanaroff-Riley type I low luminosity radio galaxies inhabit regions of higher galaxy density than radio-quiet ellipticals and powerful radio sources, and are more luminous in the optical
    Gonzalez-Serrano, J. I. et al.

    Fecha de publicación:

    5
    1993
    Bibcode
    1993AJ....105.1710G
    Número de citas
    39
  • Sin árbitro
    Supernova 1993J in NGC 3031
    IAUC 5795 available at Central Bureau for Astronomical Telegrams. IAUC 5795 available at Central Bureau for Astronomical Telegrams.
    Kidger, M. et al.

    Fecha de publicación:

    5
    1993
    Bibcode
    1993IAUC.5795....2K
    Número de citas
    3
  • Con árbitro
    Steps toward determination of the size and structure of the broad-line region in active galactic nuclei. IV - Intensity variations of the optical emission lines of NGC 5548
    Measurements of optical emission-line flux variations based on spectra of the Seyfert galaxy NGC 5548 obtained between December 1988 and October 1989 are reported. All of the measured optical emission lines, H-alpha, H-beta, H-gamma, He I 5876, and He II 4686, exhibit the same qualitative behavior as the UV and optical continua, but with short time
    Wills, D. et al.

    Fecha de publicación:

    5
    1993
    Bibcode
    1993ApJ...408..416D
    Número de citas
    96