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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  • The Gaia-ESO Survey: Calibrating the lithium-age relation with open clusters and associations. I. Cluster age range and initial membership selections
    Context. Previous studies of open clusters have shown that lithium depletion is not only strongly age dependent but also shows a complex pattern with other parameters that is not yet understood. For pre- and main-sequence late-type stars, these parameters include metallicity, mixing mechanisms, convection structure, rotation, and magnetic activity
    Gutiérrez Albarrán, M. L. et al.

    Fecha de publicación:

    11
    2020
    Número de citas
    38
  • The circum-galactic medium of quasars: transverse and line-of-sight absorptions
    Quasar projected pairs (QPPs) can be used for investigating the circumgalactic medium of quasars through the study of intervening absorption lines in the spectrum of the background quasar (QSO B) that are at the same redshift of the foreground quasar (QSO F). Here we report on optical spectroscopy, gathered at Gran Telescopio Canarias, of 14 QPPs
    Sandrinelli, A. et al.

    Fecha de publicación:

    11
    2020
    Número de citas
    0
  • The CARMENES search for exoplanets around M dwarfs. Three temperate-to-warm super-Earths
    We announce the discovery of two planets orbiting the M dwarfs GJ 251 (0.360 ± 0.015M ☉) and HD 238090 (0.578 ± 0.021M ☉) based on CARMENES radial velocity (RV) data. In addition, we independently confirm with CARMENES data the existence of Lalande 21185 b, a planet that has recently been discovered with the SOPHIE spectrograph. All three planets
    Stock, S. et al.

    Fecha de publicación:

    11
    2020
    Número de citas
    45
  • Spin rates of V-type asteroids
    Context. Basaltic V-type asteroids play a crucial role in studies of Solar System evolution and planetesimal formation. Comprehensive studies of their physical, dynamical, and statistical properties provide insight into these processes. Thanks to wide surveys, currently there are numerous known V-type and putative V-type asteroids, allowing a
    Oszkiewicz, Dagmara et al.

    Fecha de publicación:

    11
    2020
    Número de citas
    10
  • Spectral characterisation of 14 V-type candidate asteroids from the MOVIS catalogue
    Most of the currently known basaltic (V-type) asteroids are believed to be past or present members of the Vesta dynamical family. The rising discoveries of V-type asteroids that are not linked to the Vesta family dynamically suggest that a number of major basaltic bodies may have been present during the early stages of the solar system. Using the
    Matlovič, Pavol et al.

    Fecha de publicación:

    11
    2020
    Número de citas
    6
  • Spatially resolved measurements of the solar photospheric oxygen abundance
    Aims: We report the results of a novel determination of the solar oxygen abundance using spatially resolved observations and inversions. We seek to derive the photospheric solar oxygen abundance with a method that is robust against uncertainties in the model atmosphere. Methods: We use observations with spatial resolution obtained at the Vacuum
    Cubas Armas, M. et al.

    Fecha de publicación:

    11
    2020
    Número de citas
    7