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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  • Observational constraints on the optical and near-infrared emission from the neutron star-black hole binary merger candidate S190814bv
    Context. Gravitational wave (GW) astronomy has rapidly reached maturity, becoming a fundamental observing window for modern astrophysics. The coalescences of a few tens of black hole (BH) binaries have been detected, while the number of events possibly including a neutron star (NS) is still limited to a few. On 2019 August 14, the LIGO and Virgo
    Ackley, K. et al.

    Fecha de publicación:

    11
    2020
    Número de citas
    93
  • Open Cluster Chemical Homogeneity throughout the Milky Way
    The chemical homogeneity of surviving stellar clusters contains important clues about interstellar medium (ISM) mixing efficiency, star formation, and the enrichment history of the Galaxy. Existing measurements in a handful of open clusters suggest homogeneity in several elements at the 0.03 dex level. Here we present (i) a new cluster member
    Poovelil, Vijith Jacob et al.

    Fecha de publicación:

    11
    2020
    Número de citas
    24
  • Planck intermediate results. LVII. Joint Planck LFI and HFI data processing
    We present the NPIPE processing pipeline, which produces calibrated frequency maps in temperature and polarization from data from the Planck Low Frequency Instrument (LFI) and High Frequency Instrument (HFI) using high-performance computers. NPIPE represents a natural evolution of previous Planck analysis efforts, and combines some of the most
    Planck Collaboration et al.

    Fecha de publicación:

    11
    2020
    Número de citas
    171
  • 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
  • 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
    8
  • 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
    37