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

  • The bifurcated age-metallicity relation of Milky Way globular clusters and its implications for the accretion history of the galaxy
    We use recently derived ages for 61 Milky Way (MW) globular clusters (GCs) to show that their age-metallicity relation (AMR) can be divided into two distinct, parallel sequences at [Fe/H] ≳ -1.8. Approximately one-third of the clusters form an offset sequence that spans the full range in age (˜10.5-13 Gyr), but is more metal rich at a given age by
    Leaman, R. et al.

    Fecha de publicación:

    11
    2013
    Número de citas
    207
  • The ALHAMBRA survey: reliable morphological catalogue of 22 051 early- and late-type galaxies
    Advanced Large Homogeneous Area Medium Band Redshift Astronomical (ALHAMBRA) is photometric survey designed to trace the cosmic evolution and cosmic variance. It covers a large area of ˜4 deg2 in eight fields, where seven fields overlap with other surveys, allowing us to have complementary data in other wavelengths. All observations were carried
    Quintana, J. M. et al.

    Fecha de publicación:

    11
    2013
    Número de citas
    29
  • The (galaxy-wide) IMF in giant elliptical galaxies: from top to bottom
    Recent evidence based independently on spectral line strengths and dynamical modelling point towards a non-universal stellar initial mass function (IMF), probably implying an excess of low-mass stars in elliptical galaxies with a high velocity dispersion. Here, we show that a time-independent bottom-heavy IMF is compatible neither with the observed
    Weidner, C. et al.

    Fecha de publicación:

    11
    2013
    Número de citas
    83
  • Properties of oscillatory motions in a facular region
    Aims: We study the properties of waves in a facular region of moderate strength in the photosphere and chromosphere. Our aim is to statistically analyse the wave periods, power, and phase relations as a function of the magnetic field strength and inclination. Methods: Our work is based on observations obtained at the German Vacuum Tower Telescope
    Kostik, R. et al.

    Fecha de publicación:

    11
    2013
    Número de citas
    23
  • Propagating Waves Transverse to the Magnetic Field in a Solar Prominence
    We report an unusual set of observations of waves in a large prominence pillar that consist of pulses propagating perpendicular to the prominence magnetic field. We observe a huge quiescent prominence with the Solar Dynamics Observatory Atmospheric Imaging Assembly in EUV on 2012 October 10 and only a part of it, the pillar, which is a foot or barb
    Schmieder, B. et al.

    Fecha de publicación:

    11
    2013
    Número de citas
    62
  • Probing the Upper Scorpius mass function in the planetary-mass regime
    We present the results of a deep ZYJ near-infrared survey of 13.5 deg2 in the Upper Scorpius (USco) OB association. We photometrically selected ˜100 cluster member candidates with masses in the range of 30-5 Jupiters, according to state-of-the-art evolutionary models. We identified 67 ZYJ candidates as bona fide members, based on complementary
    Lodieu, N. et al.

    Fecha de publicación:

    11
    2013
    Número de citas
    25