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

  • APOGEE [C/N] Abundances Across the Milky Way
    The Apache Point Observatory Galactic Evolution Experiment (APOGEE) provides precise carbon and nitrogen abundances for over 100,000 red giant stars across the Milky Way Galaxy (MW). Recently, it has been shown that the carbon-to-nitrogen ratio (often expressed as [C/N]) can be indicative of the mass of a red giant star, from which an age can be
    Hasselquist, S. et al.

    Fecha de publicación:

    1
    2018
    Número de citas
    0
  • An UXor among FUors: Extinction-related Brightness Variations of the Young Eruptive Star V582 Aur
    V582 Aur is an FU Ori-type young eruptive star in outburst since ∼1985. The eruption is currently in a relatively constant plateau phase, with photometric and spectroscopic variability superimposed. Here we will characterize the progenitor of the outbursting object, explore its environment, and analyze the temporal evolution of the eruption. We are
    Ábrahám, P. et al.

    Fecha de publicación:

    1
    2018
    Número de citas
    26
  • An excess of massive stars in the local 30 Doradus starburst
    The 30 Doradus star-forming region in the Large Magellanic Cloud is a nearby analog of large star-formation events in the distant universe. We determined the recent formation history and the initial mass function (IMF) of massive stars in 30 Doradus on the basis of spectroscopic observations of 247 stars more massive than 15 solar masses (M☉). The
    Schneider, F. R. N. et al.

    Fecha de publicación:

    1
    2018
    Número de citas
    218
  • A HST/WFC3 Search for Substellar Companions in the Orion Nebula Cluster
    We present new results relative to the population of substellar binaries in the Orion Nebula Cluster. We reprocessed HST/WFC3 data using an analysis technique developed to detect close companions in the wings of the stellar PSFs, based on the PyKLIP implementation of the KLIP PSF subtraction algorithm. Starting from a sample of ~1200 stars selected
    Strampelli, G. M. et al.

    Fecha de publicación:

    1
    2018
    Número de citas
    0
  • A dusty star-forming galaxy at z = 6 revealed by strong gravitational lensing
    Since their discovery, submillimetre-selected galaxies1,2 have revolutionized the field of galaxy formation and evolution. From the hundreds of square degrees mapped at submillimetre wavelengths3-5, only a handful of sources have been confirmed to lie at z > 5 (refs 6-10) and only two at z ≥ 6 (refs 11,12). All of these submillimetre galaxies are
    Zavala, J. A. et al.

    Fecha de publicación:

    1
    2018
    Número de citas
    91
  • 280 one-opposition near-Earth asteroids recovered by the EURONEAR with the Isaac Newton Telescope
    Context. One-opposition near-Earth asteroids (NEAs) are growing in number, and they must be recovered to prevent loss and mismatch risk, and to improve their orbits, as they are likely to be too faint for detection in shallow surveys at future apparitions. Aims: We aimed to recover more than half of the one-opposition NEAs recommended for
    Vaduvescu, O. et al.

    Fecha de publicación:

    1
    2018
    Número de citas
    14