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

  • Hint of an exocomet transit in the CHEOPS light curve of HD 172555
    HD 172555 is a young (~20 Myr) A7V star surrounded by a 10 au wide debris disk suspected to be replenished partly by collisions between large planetesimals. Small evaporating transiting bodies, that is exocomets, have also been detected in this system by spectroscopy. After β Pictoris, this is another example of a system possibly witnessing a phase
    Kiefer, F. et al.

    Fecha de publicación:

    3
    2023
    Número de citas
    12
  • Hidden depths in the local Universe: The Stellar Stream Legacy Survey
    Context. Mergers and tidal interactions between massive galaxies and their dwarf satellites are a fundamental prediction of the Lambda-cold dark matter cosmology. These events are thought to provide important observational diagnostics of non-linear structure formation. Stellar streams in the Milky Way and Andromeda are spectacular evidence for
    Martínez-Delgado, David et al.

    Fecha de publicación:

    3
    2023
    Número de citas
    68
  • Glancing through the debris disk: Photometric analysis of DE Boo with CHEOPS
    Aims: DE Boo is a unique system, with an edge-on view through the debris disk around the star. The disk, which is analogous to the Kuiper belt in the Solar System, was reported to extend from 74 to 84 AU from the central star. The high photometric precision of the Characterising Exoplanet Satellite (CHEOPS) provided an exceptional opportunity to
    Rando, N. et al.

    Fecha de publicación:

    3
    2023
    Número de citas
    2
  • Gaia-ESO survey: Massive stars in the Carina Nebula. I. A new census of OB stars
    Context. The Carina Nebula is one of the major massive star-forming regions in the Galaxy. Its relatively nearby distance (2.35 kpc) makes it an ideal laboratory for the study of massive star formation, structure, and evolution, both for individual stars and stellar systems. Thanks to the high-quality spectra provided by the Gaia-ESO survey and the
    Berlanas, S. R. et al.

    Fecha de publicación:

    3
    2023
    Número de citas
    12
  • Forming intracluster gas in a galaxy protocluster at a redshift of 2.16
    Galaxy clusters are the most massive gravitationally bound structures in the Universe, comprising thousands of galaxies and pervaded by a diffuse, hot intracluster medium (ICM) that dominates the baryonic content of these systems. The formation and evolution of the ICM across cosmic time 1 is thought to be driven by the continuous accretion of
    Di Mascolo, Luca et al.

    Fecha de publicación:

    3
    2023
    Número de citas
    53
  • Formation and evolution of carbonaceous asteroid Ryugu: Direct evidence from returned samples
    Samples of the carbonaceous asteroid Ryugu were brought to Earth by the Hayabusa2 spacecraft. We analyzed seventeen Ryugu samples measuring 1-8 mm. CO2-bearing water inclusions are present within a pyrrhotite crystal, indicating that Ryugu’s parent asteroid formed in the outer Solar System. The samples contain low abundances of materials that
    Nakamura T. et al. et al.

    Fecha de publicación:

    3
    2023
    Número de citas
    58