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

  • Sin árbitro
    Mapping Galaxy Clusters in the Distant Universe
    We present the science case for mapping several thousand galaxy (proto)clusters at z=1-10 with a large aperture single dish sub-mm facility, producing a high-redshift counterpart to local large surveys of rich clusters like the well-studied Abell catalogue.
    Dannerbauer, Helmut et al.

    Fecha de publicación:

    5
    2019
    Bibcode
    2019BAAS...51c.293D
    Número de citas
    3
  • Con árbitro
    MAGIC and Fermi-LAT gamma-ray results on unassociated HAWC sources
    The HAWC Collaboration released the 2HWC catalogue of TeV sources, in which 19 show no association with any known high-energy (HE; E ≳ 10 GeV) or very-high-energy (VHE; E ≳ 300 GeV) sources. This catalogue motivated follow-up studies by both the Major Atmospheric Gamma-ray Imaging Cherenkov (MAGIC) and Fermi-LAT (Large Area Telescope) observatories
    Ahnen, M. L. et al.

    Fecha de publicación:

    5
    2019
    Bibcode
    2019MNRAS.485..356A
    Número de citas
    7
  • Con árbitro
    Lower atmosphere and pressure evolution on Pluto from ground-based stellar occultations, 1988-2016
    Context. The tenuous nitrogen (N2) atmosphere on Pluto undergoes strong seasonal effects due to high obliquity and orbital eccentricity, and has recently (July 2015) been observed by the New Horizons spacecraft. Aims: The main goals of this study are (i) to construct a well calibrated record of the seasonal evolution of surface pressure on Pluto
    Meza, E. et al.

    Fecha de publicación:

    5
    2019
    Bibcode
    2019A&A...625A..42M
    Número de citas
    35
  • Con árbitro
    Low-frequency gravity waves in blue supergiants revealed by high-precision space photometry
    Almost all massive stars explode as supernovae and form a black hole or neutron star. The remnant mass and the impact of the chemical yield on subsequent star formation and galactic evolution strongly depend on the internal physics of the progenitor star, which is currently not well understood. The theoretical uncertainties of stellar interiors
    Bowman, Dominic M. et al.

    Fecha de publicación:

    5
    2019
    Bibcode
    2019NatAs...3..760B
    Número de citas
    141