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

  • Dynamics of early-type dwarf galaxies in the Virgo Cluster - a SAURON perspective
    Not Available
    Ryś, Agnieszka

    Fecha de publicación:

    6
    2011
    Número de citas
    0
  • Color-Magnitude Diagrams, Probabilistic Synthesis Models and the Upper Mass Limit of the Initial Mass Function
    We present the underlying relations between color-magnitude diagrams (CMDs) and synthesis models through the use of stellar luminosity distribution functions. CMD studies make direct use of the stellar luminosity distribution function while, in general, synthesis models only use its mean value, even though high-order moments can also be obtained
    Cerviño, M. et al.

    Fecha de publicación:

    6
    2011
    Número de citas
    4
  • Clear detection of dusty torus signatures in a weak-line radio galaxy: the case of PKS 0043-42
    We report the clearest detection to date of dusty torus signatures in a weak-line radio galaxy (WLRG). The deep Spitzer InfraRed Spectrograph (IRS) rest-frame mid-infrared (MIR) spectrum of the WLRG PKS 0043-42 (z= 0.116) shows a clear spectral turnover at λ≳ 20 μs suggestive of warm dust, as well as a 9.7-μm silicate absorption feature. In
    Ramos-Almeida, C. et al.

    Fecha de publicación:

    6
    2011
    Número de citas
    13
  • Blue not brown: UKIRT Infrared Deep Sky Survey T dwarfs with suppressed K-band flux
    We have used blue near-infrared colours to select a group of 12 spectroscopically confirmed United Kingdom InfraRed Telescope (UKIRT) Infrared Deep Sky Survey (UKIDSS) T dwarfs later than T4. From amongst these, we identify the first two kinematic halo T-dwarf candidates. Blue near-infrared colours have been attributed to collisionally induced
    Murray, D. N. et al.

    Fecha de publicación:

    6
    2011
    Número de citas
    51
  • Beryllium abundances in stars with planets. Extending the sample
    Context. Chemical abundances of light elements such as beryllium in planet-host stars allow us to study the planet formation scenarios and/or investigate possible surface pollution processes. Aims: We present here an extension of previous beryllium abundance studies. The complete sample consists of 70 stars that host planets and 30 stars without
    Gálvez-Ortiz, M. C. et al.

    Fecha de publicación:

    6
    2011
    Número de citas
    12