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

  • Gaia FGK benchmark stars: abundances of α and iron-peak elements
    Context. In the current era of large spectroscopic surveys of the Milky Way, reference stars for calibrating astrophysical parameters and chemical abundances are of paramount importance. Aims: We determine elemental abundances of Mg, Si, Ca, Sc, Ti, V, Cr, Mn, Co, and Ni for our predefined set of Gaia FGK benchmark stars. Methods: By analysing high
    Jofré, P. et al.

    Fecha de publicación:

    10
    2015
    Número de citas
    142
  • Galactic Bulges and Inner Disks, as Seen by SAURON
    We discuss SAURON integral field observations of a sample of 42 spirals, ranging in type from Sa to Sd. Using 2D maps of the stellar velocity, velocity dispersion, and absorption line strength, it is now much easier to understand the nature of nearby galactic bulges and inner disks. Here we briefly present some of our results.
    Peletier, R. F. et al.

    Fecha de publicación:

    10
    2008
    Número de citas
    0
  • Galactic population of radio and gamma-ray pulsars
    We simulate the characteristics of the Galactic population of radio and gamma-ray pulsars using Monte Carlo techniques. At birth, neutron stars are spatially distributed with supernova-kick velocities in the Galactic disk and randomly dispersed in age back to 109 years. They are evolved in the Galactic gravitational potential to the present time
    Gonthier, Peter L. et al.

    Fecha de publicación:

    10
    2001
    Número de citas
    0
  • Galactic Population of Radio and Gamma-Ray Pulsars
    We simulate the characteristics of the Galactic population of radio and gamma-ray pulsars using Monte Carlo techniques. At birth, neutron stars are spatially distributed with supernova-kick velocities in the Galactic disk and randomly dispersed in age back to 109 years. They are evolved in the Galactic gravitational potential to the present time
    Gonthier, P. L. et al.

    Fecha de publicación:

    10
    2000
    Número de citas
    0
  • Galactic population of radio and gamma-ray pulsars
    We simulate the characteristics of the Galactic population of radio and gamma-ray pulsars using Monte Carlo techniques. At birth, neutron stars are spatially distributed with supernova-kick velocities in the Galactic disk and randomly dispersed in age over the past 109 years. From their birth location, the neutron stars are evolved in the Galactic
    Gonthier, Peter L. et al.

    Fecha de publicación:

    10
    2001
    Número de citas
    0