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

  • X-Ray Nature of the LINER Nuclear Sources
    We have investigated the nature of the energy source of 36 LINERs with Chandra X-ray observations selected from the catalogue by Carrillo et al. (1999). In most galaxies a nuclear compact source has been detected in the hard band (2-8 KeV). However they show a rather irregular morphology embedded in diffuse X-ray emission for lower energies (0.3-2
    González-Martin, O. et al.

    Fecha de publicación:

    0
    2005
    Número de citas
    0
  • Wrinkles in the Galaxy
    New calculations of the Galactic contribution to microwave background radiation anisotropies are carried out and a probable Galactic predominance over cosmological signals at large scales is explored for these frequencies When we take into account a frequency-dependent contrast of molecular cloud with respect to the Galactic background of the
    López-Corredoira, Martín

    Fecha de publicación:

    0
    2005
    Número de citas
    0
  • VSA observations of the Sunyaev-Zel'dovich effect in galaxy clusters and in the Corona Borealis supercluster
    Not Available
    Genova-Santos, R. et al.

    Fecha de publicación:

    0
    2005
    Número de citas
    1
  • Voigt a-damping parameter of the spectral lines emitted by a plasma flame and a plasma column generated by a microwave at atmospheric pressure
    Atomic emission spectroscopy is a passive spectroscopy technique widely used in the diagnosis of plasmas which does not alter the internal kinectic of the discharge during the measurement process, under high pressure conditions. Line profiles are adequately fitted by a Voigt function. One of the parameter which characterizes these spectral lines is
    Santiago, I. et al.

    Fecha de publicación:

    0
    2005
    Número de citas
    0