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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  • Images at the Highest Angular Resolution with GRAVITY: The Case of η Carinae
    The main goal of an interferometer is to probe the physics of astronomical objects at the highest possible angular resolution. The most intuitive way of doing this is by reconstructing images from the interferometric data. GRAVITY at the Very Large Telescope Interferometer (VLTI) has proven to be a fantastic instrument in this endeavour. In this
    GRAVITY Collaboration et al.

    Fecha de publicación:

    12
    2019
    Número de citas
    1
  • Hunting Exoplanets with Single-Mode Optical Interferometry
    The GRAVITY instrument was primarily conceived for imaging and astrometry of the Galactic centre. However, its sensitivity and astrometric capabilities have also enabled interferometry to reach a new domain of astrophysics: exoplanetology. In March 2019, the GRAVITY collaboration published the first spectrum and astrometry of an exoplanet obtained
    GRAVITY Collaboration et al.

    Fecha de publicación:

    12
    2019
    Número de citas
    2
  • High-frequency Wave Propagation Along a Spicule Observed by CLASP
    The Chromospheric Lyman-Alpha Spectro-Polarimeter (CLASP) sounding rocket experiment, launched in 2015 September, observed the hydrogen Lyα line (121.6 nm) in an unprecedented high temporal cadence of 0.3 s. CLASP performed sit-and-stare observations of the quiet Sun near the limb for 5 minutes with a slit perpendicular to the limb and successfully
    Yoshida, Masaki et al.

    Fecha de publicación:

    12
    2019
    Número de citas
    8
  • H α morphologies of star clusters: a LEGUS study of H II region evolution time-scales and stochasticity in low-mass clusters
    The morphology of H II regions around young star clusters provides insight into the time-scales and physical processes that clear a cluster's natal gas. We study ̃700 young clusters (≤10 Myr) in three nearby spiral galaxies (NGC 7793, NGC 4395, and NGC 1313) using Hubble Space Telescope (HST) imaging from LEGUS (Legacy ExtraGalactic Ultraviolet
    Hannon, Stephen et al.

    Fecha de publicación:

    12
    2019
    Número de citas
    55
  • Growth and disruption in the Lyra complex
    Context. Nearby clusters of galaxies, z ≲ 0.1, are cosmic structures still under formation. Understanding the thermodynamic properties of merging clusters can provide crucial information on how they grow in the local universe. Aims: A detailed study of the intra-cluster medium (ICM) properties of un-relaxed systems is essential to understand the
    Clavico, S. et al.

    Fecha de publicación:

    12
    2019
    Número de citas
    8
  • GRAVITY and the Galactic Centre
    On a clear night, our home galaxy, the Milky Way, is visible as a starry ribbon across the sky. Its core is located in the constellation of Sagittarius, approximately where the bright glow is interrupted by the darkest dust filaments. There, hidden, lies a massive black hole. To peer through the obscuring clouds and see the stars and gas near the
    GRAVITY Collaboration et al.

    Fecha de publicación:

    12
    2019
    Número de citas
    2