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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  • Stellar Populations and Kinematics of Red Galaxies at z > 2: Implications for the Formation of Massive Galaxies
    We recently identified a substantial population of galaxies at z>2 with comparatively red rest-frame optical colors. These distant red galaxies (DRGs) are efficiently selected by the simple observed color criterion Js-Ks>2.3. In this paper we present near-infrared spectroscopy with Keck NIRSPEC of six DRGs with previously measured redshifts 2.4
    van Dokkum, Pieter G. et al.

    Fecha de publicación:

    8
    2004
    Número de citas
    149
  • Stellar Populations and the Local Group Membership of the Dwarf Galaxy DDO 210
    We present deep BVI CCD photometry of the stars in the dwarf galaxy DDO 210. The color-magnitude diagrams of DDO 210 show a well-defined red giant branch (RGB) and a blue plume. The tip of the RGB is found to be at I_TRGB=20.95+/-0.10 mag. From this, the distance to DDO 210 is estimated to be d=950+/-50 kpc. The corresponding distance of DDO 210 to
    Lee, Myung Gyoon et al.

    Fecha de publicación:

    8
    1999
    Número de citas
    49
  • Stellar Populations Gradients in Isolated Dwarf Galaxies
    We present the star formation history (SFH) as a function of galactocentric radius for a sample of isolated dwarf galaxies from the Local Cosmology from the Isolated Dwarfs (LCID) project. The results show a decrease of the star formation with radius for stars with ages ≤ 9 Gyr. Star formation for ages ≥ 10 Gyr is present regardless of distance to
    Hidalgo, S. L. et al.

    Fecha de publicación:

    8
    2012
    Número de citas
    1
  • Stellar Populations in the Outskirts of the Small Magellanic Cloud: No Outer Edge Yet
    We report the detection of intermediate-age and old stars belonging to the SMC at 6.5 kpc from the SMC center in the southern direction. We show, from the analysis of three high-quality 34'×33' CMDs, that the age composition of the stellar population is similar at galactocentric distances of ~4.7, ~5.6, and ~6.5 kpc. The surface brightness profile
    Noël, Noelia E. D. et al.

    Fecha de publicación:

    8
    2007
    Número de citas
    34