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

  • Dust in active galactic nuclei. Mid-infrared T-ReCS/Gemini spectra using the new RedCan pipeline
    Context. The unified model of active galactic nuclei (AGN) claims that the properties of AGN depend on the viewing angle of the observer with respect to a toroidal distribution of dust surrounding the nucleus. Both the mid-infrared (MIR) attenuation and continuum luminosity are expected to be related to dust associated with the torus. Therefore
    González-Martín, O. et al.

    Fecha de publicación:

    5
    2013
    Número de citas
    84
  • Distinct stellar populations in the inner bars of double-barred galaxies
    Numerical simulations of double-barred galaxies predict the build-up of different structural components (e.g. bulges, inner discs) in the central regions of disc galaxies. In those simulations, inner bars have a prominent role in the internal secular evolution of their host galaxies. The development of bulges and inner discs is, however, poorly
    de Lorenzo-Cáceres, A. et al.

    Fecha de publicación:

    5
    2013
    Número de citas
    41
  • DETAILED STELLAR POPULATION ANALYSIS OF EARLY-TYPE GALAXIES WITH REDSHIFT TO CONSTRAIN THEIR EVOLUTION
    Una de las cuestiones básicas de la Astronomía moderna es cómo las galaxias de las diferentes familias han evolucionado desde su formación. Una de estas familias, las galaxias de tipos tempranos (ETGs, del inglés Early-Type Galaxy), formadas por galaxias elípticas y lenticulares y que contienen la mayor parte de la materia luminosa del Universo, ha
    Anna Ferré Mateu

    Fecha de publicación:

    5
    2013
  • Deriving the dynamical masses of Ultra-Luminous X-ray Sources with OSIRIS
    Ultra Luminous X-ray Sources (ULXs) are extragalactic X-ray point sources with L_X ˜ 10^39-10^41 erg s^-1 discovered in the 80s with the Einstein satellite and confirmed as black hole X-ray binaries during the last decade. The nature of the compact object is highly controversial. They could be super-Eddington stellar-mass black holes or
    González-Galán, A. et al.

    Fecha de publicación:

    5
    2013
    Número de citas
    0
  • Deep Blank Fields for the GTC
    The use of deep blank fields is crucial for the correct operation of the GTC. Hitherto, the list of deepest blank fields was the compilation by M. Azzaro for the ING telescope. However, they demonstrated to be shallow for large class telescopes. We used TESELA, a new VO tool, to determine blank fields for their use with OSIRIS at the GTC. The
    Jiménez-Esteban, F. et al.

    Fecha de publicación:

    5
    2013
    Número de citas
    0
  • Deep blank field catalogue for medium- and large-size telescopes
    Taking advantage of the Virtual Observatory, we have searched for deep blank fields (DBFs) throughout the whole sky, with a minimum size of 10' diameter and an increasing threshold magnitude from 15 to 18 in USNO-B R band. The result is the catalogue with the deepest blank fields known so far. Some of them have been tested with the 10.4m GTC
    Jiménez-Esteban, F. M. et al.

    Fecha de publicación:

    5
    2013
    Número de citas
    0