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
    The Fundamental Plane of Radio Galaxies
    The global properties of early-type galaxies are fairly well described through a linear relation (the Fundamental Plane, FP [2],[3]) in the space defined by three observables: the effective radius r e, the average surface brightness μ_e and the central velocity dispersion σ_c. The FP has been shown to be close to the plane defining the virial
    Bettoni, Daniela et al.

    Fecha de publicación:

    0
    2003
    Bibcode
    2003mglh.conf..154B
    Número de citas
    0
  • Sin árbitro
    The Effects of Transition Time on the Populations of Post-AGB Stars and on the Nebular Evolution
    Not Available
    Villaver, E. et al.

    Fecha de publicación:

    0
    2003
    Bibcode
    2003IAUS..209..133V
    Número de citas
    0
  • Sin árbitro
    The Dynamical Gas Evolution of Low-and Intermediate-Mass Stars: PN Formation
    Not Available
    Villaver, E. et al.

    Fecha de publicación:

    0
    2003
    Bibcode
    2003IAUS..209..155V
    Número de citas
    0
  • Sin árbitro
    The diffuse ionized gas in galaxies
    An investigation of the diffuse ionized gas (DIG) and its underlying physical processes is the focal point of this study. We aim to survey the prevalence, morphology, distribution, and luminosity of the DIG as well as its variations with galaxy morphology.
    Rozas, M. et al.

    Fecha de publicación:

    0
    2003
    Bibcode
    2003RMxAC..16..308R
    Número de citas
    0
  • Sin árbitro
    The Development of Stellar Photometric Standards for ISO.
    The ISO ground-based preparatory programme working group (ISO-GBPPwg) was set the goal in 1990 to characterise accurately in the infrared some 400 stars covering the whole sky. Telescopes in Chile, Hawaii and the Canary Islands were used to obtain J, H, K, and L photometry for all of these stars and, for the brightest ones, spectroscopy and/or N
    Hammersley, P. L. et al.

    Fecha de publicación:

    0
    2003
    Bibcode
    2003ESASP.481..129H
    Número de citas
    6