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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  • Deep Near-Infrared Mapping of Young and Old Stars in Blue Compact Dwarf Galaxies
    We analyze J, H, and Ks near-infrared data for nine blue compact dwarf (BCD) galaxies, selected from a larger sample that we have already studied in the optical. We present contour maps, surface brightness and color profiles, and color maps of the sample galaxies. The morphology of the BCDs in the near-infrared (NIR) has been found to be basically
    Cairós, Luz M. et al.

    Fecha de publicación:

    8
    2003
    Número de citas
    59
  • A far-infrared view of the Lockman Hole from ISO 95-μm observations - I. A new data reduction method
    We report results from a new analysis of a deep 95-μm imaging survey with the photopolarimeter ISOPHOT on-board the Infrared Space Observatory, over a 40 × 40 arcmin2 area within the Lockman Hole. To this end we exploit a newly developed parametric algorithm able to identify and clean spurious signals induced by cosmic rays impacts and by transient
    Rodighiero, G. et al.

    Fecha de publicación:

    8
    2003
    Número de citas
    22
  • Wavelength Dependence of Pulsation Amplitudes in DBV White Dwarfs
    Not Available
    Weidner, C. et al.

    Fecha de publicación:

    7
    2003
    Número de citas
    0
  • Varying Galactic-field Stellar IMF through Clustered Star Formation
    Not Available
    Weidner, Carsten et al.

    Fecha de publicación:

    7
    2003
    Número de citas
    0
  • Using globular clusters to test gravity in the weak acceleration regime
    We have carried out a study of the velocity dispersion of the stars in the outskirts of the globular cluster omega Cen, finding that the velocity dispersion remains constant at large radii rather than decrease monotonically. The dispersion starts to be constant for an acceleration of gravity of a=2.1+0.5-0.4x 10-8 cm s-2. A similar result is
    Scarpa, R. et al.

    Fecha de publicación:

    7
    2003
    Número de citas
    52