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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  • 3D kinematics through the X-shaped Milky Way bulge
    Context. It has recently been discovered that the Galactic bulge is X-shaped, with the two southern arms of the X both crossing the lines of sight at l = 0 and | b| > 4, hence producing a double red clump in the bulge color magnitude diagram. Dynamical models predict the formation of X-shaped bulges as extreme cases of boxy-peanut bulges. However
    Vásquez, S. et al.

    Fecha de publicación:

    7
    2013
    Número de citas
    57
  • BÚSQUEDA DE LA MATERIA BARIÓNICA EN EL SUPERCÚMULO DE CORONA BOREALIS
    Uno de los parámetros mas relevantes en la descripción del Universo es la densidad bariónica media. Esta ha sido estimada a través de las abundancias de los elementos primordiales y confirmada en estudios recientes del espectro de potencias del Fondo Cósmico de Microondas (FCM). Sin embargo, las observaciones de la materia bariónica en el universo
    Carmen Pilar Padilla Torres

    Fecha de publicación:

    7
    2013
  • Winds of Very Low Metallicity OB Stars: Beyond the Magellanic Clouds
    Very low metallicity massive stars are a key piece to understanding the infant, extremely metal-poor Universe and its early development. Our models for these objects rely to a great extent on the theory of radiation driven winds, important agents of stellar evolution and feedback. However, the theory of radiation driven winds has only been
    Garcia, M. et al.

    Fecha de publicación:

    6
    2013
    Número de citas
    0
  • Very Low Mass Stellar and Substellar Companions to Solar-like Stars from MARVELS. V. A Low Eccentricity Brown Dwarf from the Driest Part of the Desert, MARVELS-6b
    We describe the discovery of a likely brown dwarf (BD) companion with a minimum mass of 31.7 ± 2.0 M Jup to GSC 03546-01452 from the MARVELS radial velocity survey, which we designate as MARVELS-6b. For reasonable priors, our analysis gives a probability of 72% that MARVELS-6b has a mass below the hydrogen-burning limit of 0.072 M ☉, and thus it is
    De Lee, Nathan et al.

    Fecha de publicación:

    6
    2013
    Número de citas
    21
  • V2492 Cyg light variations (Kospal+, 2013)
    We obtained optical and near-infrared images with VRIJHKs filters between 2010 September 19 and 2012 October 12 using four telescopes: the Schmidt and RCC telescopes of the Konkoly Observatory (Hungary), as well as the IAC-80 and Telescopio Carlos Sanchez (TCS) telescopes of the Teide Observatory in the Canary Islands (Spain). We observed V2492 Cyg
    Kospal, A. et al.

    Fecha de publicación:

    6
    2013
    Número de citas
    0
  • The rapid assembly of an elliptical galaxy of 400 billion solar masses at a redshift of 2.3
    Stellar archaeology shows that massive elliptical galaxies formed rapidly about ten billion years ago with star-formation rates of above several hundred solar masses per year. Their progenitors are probably the submillimetre bright galaxies at redshifts z greater than 2. Although the mean molecular gas mass (5×1010 solar masses) of the
    Fu, Hai et al.

    Fecha de publicación:

    6
    2013
    Número de citas
    130