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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  • Oscillation mode frequencies of 61 main-sequence and subgiant stars observed by Kepler
    Context. Solar-like oscillations have been observed by Kepler and CoRoT in several solar-type stars, thereby providing a way to probe the stars using asteroseismology Aims: We provide the mode frequencies of the oscillations of various stars required to perform a comparison with those obtained from stellar modelling. Methods: We used a time series
    Appourchaux, T. et al.

    Fecha de publicación:

    7
    2012
    Número de citas
    139
  • Non-local thermodynamic equilibrium inversions from a 3D magnetohydrodynamic chromospheric model
    Context. The structure of the solar chromosphere is believed to be governed by magnetic fields, even in quiet-Sun regions that have a relatively weak photospheric field. During the past decade inversion methods have emerged as powerful tools for analyzing the chromosphere of active regions. The applicability of inversions to infer the
    de la Cruz Rodríguez, J. et al.

    Fecha de publicación:

    7
    2012
    Número de citas
    86
  • New Isolated Planetary-mass Objects and the Stellar and Substellar Mass Function of the σ Orionis Cluster
    We report on our analysis of the VISTA Orion ZY JHKs photometric data (completeness magnitudes of Z = 22.6 and J = 21.0 mag) focusing on a circular area of 2798.4 arcmin2 around the young σ Orionis star cluster (~3 Myr, ~352 pc, and solar metallicity). The combination of the VISTA photometry with optical, WISE and Spitzer data allows us to identify
    Peña-Ramírez, K. et al.

    Fecha de publicación:

    7
    2012
    Número de citas
    119
  • Multi-conjugate AO for the European Solar Telescope
    The European Solar Telescope (EST) will be a 4-meter diameter world-class facility, optimized for studies of the magnetic coupling between the deep photosphere and upper chromosphere. It will specialize in high spatial resolution observations and therefore it has been designed to incorporate an innovative built-in Multi-Conjugate Adaptive Optics
    Le Louarn, M. et al.

    Fecha de publicación:

    7
    2012
    Número de citas
    1
  • MIUSCAT: extended MILES spectral coverage - II. Constraints from optical photometry
    In this work, we show a comprehensive comparison of our new stellar population synthesis (SPS) MIUSCAT models with photometric data of globular clusters (GCs) and early-type galaxies.The models compare remarkably well with the colours of Milky Way GCs in the optical range. Likewise, the colours of M31 GCs can also be explained by the models by
    Ricciardelli, E. et al.

    Fecha de publicación:

    7
    2012
    Número de citas
    62
  • MIUSCAT: extended MILES spectral coverage - I. Stellar population synthesis models
    We extend the spectral range of our stellar population synthesis models based on the MILES and CaT empirical stellar spectral libraries. For this purpose, we combine these two libraries with the Indo-U.S. to construct composite stellar spectra to feed our models. The spectral energy distributions (SEDs) computed with these models and the originally
    Vazdekis, A. et al.

    Fecha de publicación:

    7
    2012
    Número de citas
    277