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

  • Con árbitro
    Observing the Dark Matter Density Profile of Isolated Galaxies
    Using the Sloan Digital Sky Survey (SDSS), we probe the halo mass distribution by studying the velocities of satellites orbiting isolated galaxies. In a subsample that covers 2500 deg2 on the sky, we detect about 3000 satellites with absolute blue magnitudes going down to MB=-14; most of the satellites have MB=-16 to -18, comparable to the
    Prada, Francisco et al.

    Fecha de publicación:

    11
    2003
    Bibcode
    2003ApJ...598..260P
    Número de citas
    199
  • Sin árbitro
    OJ 287
    IAUC 6104 available at Central Bureau for Astronomical Telegrams. IAUC 6104 available at Central Bureau for Astronomical Telegrams.
    Fiorucci, M. et al.

    Fecha de publicación:

    11
    1994
    Bibcode
    1994IAUC.6104....2F
    Número de citas
    7
  • Con árbitro
    Old Main-Sequence Turnoff Photometry in the Small Magellanic Cloud. II. Star Formation History and its Spatial Gradients
    We present a quantitative analysis of the star formation history (SFH) of 12 fields in the Small Magellanic Cloud (SMC) based on unprecedented deep [(B - R), R] color-magnitude diagrams (CMDs). Our fields reach down to the oldest main-sequence turnoff with a high photometric accuracy, which is vital for obtaining accurate SFHs, particularly at
    Noël, Noelia E. D. et al.

    Fecha de publicación:

    11
    2009
    Bibcode
    2009ApJ...705.1260N
    Número de citas
    66
  • Con árbitro
    Old stellar Galactic disc in near-plane regions according to 2MASS: Scales, cut-off, flare and warp
    We have pursued two different methods to analyze the old stellar population near the Galactic plane, using data from the 2MASS survey. The first method is based on the isolation of the red clump giant population in the color-magnitude diagrams and the inversion of its star counts to obtain directly the density distribution along the line of sight
    López-Corredoira, M. et al.

    Fecha de publicación:

    11
    2002
    Bibcode
    2002A&A...394..883L
    Número de citas
    249