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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  • Extremely metal-poor galaxies: The H I content
    Context. Extremely metal-poor (XMP) galaxies are chemically, and possibly dynamically, primordial objects in the local Universe. Aims: Our objective is to characterize the H i content of the XMP galaxies as a class, using as a reference the list of 140 known local XMPs compiled by Morales-Luis et al. (2011). Methods: We have observed 29 XMPs, which
    Filho, M. E. et al.

    Fecha de publicación:

    10
    2013
    Número de citas
    49
  • Discovery of the Broad-lined Type Ic SN 2013cq Associated with the Very Energetic GRB 130427A
    Long-duration gamma-ray bursts (GRBs) at z 1 are found in most cases to be accompanied by bright, broad-lined Type Ic supernovae (SNe Ic-BL). The highest-energy GRBs are mostly located at higher redshifts, where the associated SNe are hard to detect observationally. Here, we present early and late observations of the optical counterpart of the
    de Ugarte Postigo, A. et al.

    Fecha de publicación:

    10
    2013
    Número de citas
    120
  • Discovery of a planetary nebula surrounding the symbiotic star DT Serpentis
    We report the discovery of a planetary nebula centered on the poorly studied symbiotic binary star DT Ser. In a few other symbiotic stars spatially resolved nebulae have been discovered as well, but only one of them probably is a genuine planetary nebula, while the others are likely to originate in complex mass-ejection episodes from the
    Munari, U. et al.

    Fecha de publicación:

    10
    2013
    Número de citas
    8
  • Differential asteroseismic study of seismic twins observed by CoRoT. Comparison of HD 175272 with HD 181420
    Context. The CoRoT short asteroseismic runs give us the opportunity to observe a large variety of late-type stars through their solar-like oscillations. We report the observation and modeling of the F5V star HD 175272. Aims: Our aim is to define a method for extracting as much information as possible from a noisy oscillation spectrum. Methods: We
    Ozel, N. et al.

    Fecha de publicación:

    10
    2013
    Número de citas
    10
  • Combining visible-to-near-infrared spectra and WISE data of Hildas and Jupiter Trojans: preliminary results
    The Hilda asteroid group and Jupiter Trojans (JTs) are populations of primitive minor bodies whose origins have not been conclusively determined. In the framework of the so-called Nice Model, they are icy bodies scattered from the Kuiper Belt in an early epoch of the Solar System (the Late Heavy Bombardment) and finally trapped in the stable
    Ali-Lagoa, V. et al.

    Fecha de publicación:

    10
    2013
    Número de citas
    0
  • Chemical Evolution and the Galactic Habitable Zone of M31
    We have computed the Galactic Habitable Zones (GHZs) of the Andromeda galaxy (M31) based on the probability of terrestrial planet formation, which depends on the metallicity (Z) of the interstellar medium, and the number of stars formed per unit surface area. The GHZ was obtained from a chemical evolution model built to reproduce a metallicity
    Meneses-Goytia, S. et al.

    Fecha de publicación:

    10
    2013
    Número de citas
    23