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

  • Surface abundances of ON stars
    Context. Massive stars burn hydrogen through the CNO cycle during most of their evolution. When mixing is efficient or when mass transfer in binary systems occurs, chemically processed material is observed at the surface of O and B stars. Aims: ON stars show stronger lines of nitrogen than morphologically normal counterparts. Whether this
    Martins, F. et al.

    Fecha de publicación:

    6
    2015
    Número de citas
    31
  • San Pedro Mártir observations of microvariability in obscured quasars
    Fast brightness variations are a unique tool to probe the innermost regions of active galactic nuclei (AGN). These variations are called microvariability or intra-night variability, and this phenomenon has been monitored in samples of blazars and unobscured AGNs. Detecting optical microvariations in targets hidden by the obscuring torus is a
    Polednikova, J. et al.

    Fecha de publicación:

    6
    2015
    Número de citas
    1
  • Radial velocities and metallicities from infrared Ca ii triplet spectroscopy of open clusters. II. Berkeley 23, King 1, NGC 559, NGC 6603, and NGC 7245
    Context. Open clusters are key to studying the formation and evolution of the Galactic disc. However, there is a deficiency of radial velocity and chemical abundance determinations for open clusters in the literature. Aims: We intend to increase the number of determinations of radial velocities and metallicities from spectroscopy for open clusters
    Carrera, R. et al.

    Fecha de publicación:

    6
    2015
    Número de citas
    9
  • Probing the Dark Matter Radial Profile in Lens Galaxies and the Size of X-Ray Emitting Region in Quasars with Microlensing
    We use X-ray and optical microlensing measurements to study the shape of the dark matter density profile in the lens galaxies and the size of the (soft) X-ray emission region. We show that single epoch X-ray microlensing is sensitive to the source size. Our results, in good agreement with previous estimates, show that the size of the X-ray emission
    Jiménez-Vicente, J. et al.

    Fecha de publicación:

    6
    2015
    Número de citas
    39
  • Period, epoch, and prediction errors of ephemerides from continuous sets of timing measurements
    Space missions such as Kepler and CoRoT have led to large numbers of eclipse or transit measurements in nearly continuous time series. This paper shows how to obtain the period error in such measurements from a basic linear least-squares fit, and how to correctly derive the timing error in the prediction of future transit or eclipse events
    Deeg, H. J.

    Fecha de publicación:

    6
    2015
    Número de citas
    5
  • Orientatio ad sidera: astronomy and landscape in Qart Hadašt/Carthago Nova
    Archaeological investigations in Cartagena –the ancient Punic Qart Hadašt, Roman Carthago Nova– have manifested the existence of ritual, urban and topographical elements that could be analyzed from the perspective of Cultural Astronomy. Therefore, in October 2013, an interdisciplinary team of astronomers and archaeologists conducted a field
    González-García, A. C. et al.

    Fecha de publicación:

    6
    2015