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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  • The chemical composition of the Orion star forming region: stars, gas and dust
    We present a summary of main results from the studies performed in the series of papers The chemical composition of the Orion star forming region. We reinvestigate the chemical composition of B-type stars in the Orion OB1 association by means of state-of-the-art stellar atmosphere codes, atomic models and techniques, and compare the resulting
    Simón-Díaz, S. et al.

    Fecha de publicación:

    1
    2011
    Número de citas
    3
  • The Bulk of the Black Hole Growth Since z ~ 1 Occurs in a Secular Universe: No Major Merger-AGN Connection
    What is the relevance of major mergers and interactions as triggering mechanisms for active galactic nuclei (AGNs) activity? To answer this long-standing question, we analyze 140 XMM-Newton-selected AGN host galaxies and a matched control sample of 1264 inactive galaxies over z ~ 0.3-1.0 and M * 1011.7 M sun with high-resolution Hubble Space
    Cisternas, Mauricio et al.

    Fecha de publicación:

    1
    2011
    Número de citas
    355
  • The acoustic low-degree modes of the Sun measured with 14 years of continuous GOLF & VIRGO measurements
    The helioseismic Global Oscillation at Low Frequency (GOLF) and the Variability of solar Irradiance and Gravity Oscillations (VIRGO) instruments onboard SoHO, have been observing the Sun continuously for the last 14 years. In this preliminary work, we characterize the acoustic modes over the entire p-mode range in both, Doppler velocity and
    García, R. A. et al.

    Fecha de publicación:

    1
    2011
    Número de citas
    13
  • The acoustic cutoff frequency of the Sun and the solar cycle
    The acoustic cutoff frequency - highest frequency for acoustic solar eigenmodes-is an important parameter of the solar atmosphere because it determines the upper boundary of the p mode cavities. At frequencies beyond this value, acoustic disturbances are no longer trapped waves but traveling waves. Interferences amongst them, originate higher
    Jiménez, A. et al.

    Fecha de publicación:

    1
    2011
    Número de citas
    2
  • Testing Newtonian gravity with distant globular clusters: NGC 1851 and NGC 1904
    Context. Globular clusters are useful for testing the validity of Newtonian dynamics in the low acceleration regime typical of galaxies, without the complications of non-baryonic dark matter. In the absence of disturbing effects, such as tidal heating, the velocity dispersion of globular clusters is expected to vanish at large radii. If this is not
    Scarpa, R. et al.

    Fecha de publicación:

    1
    2011
    Número de citas
    54
  • Statistical structure of the atmospheric optical turbulence at Teide Observatory from recalibrated generalized SCIDAR data
    The characterization of the optical turbulence structure at an astronomical site requires a proper data base of the refractive-index structure constant, ?. Our team has been obtaining generalized SCIntillation Detection and Ranging (SCIDAR) observations to monitor ? from 2002 November-2009 January at Teide Observatory (Tenerife, Canary Islands
    García-Lorenzo, B. et al.

    Fecha de publicación:

    1
    2011
    Número de citas
    17