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

  • An impressionist view of V Hydrae. When MATISSE paints asymmetric giant blobs
    Context. Asymptotic giant branch (AGB) stars enrich the interstellar medium through their mass loss. The mechanism(s) shaping the circumstellar environment of mass-losing stars is not clearly understood so far. Aims: Our purpose is to study the effect of binary companions located within the first 10 stellar radii from the primary AGB star. In this
    Planquart, L. et al.

    Fecha de publicación:

    7
    2024
    Número de citas
    3
  • An extreme ultra-diffuse galaxy with the mass of the Small Magellanic Cloud
    Extremely faint galaxies (mu_V>27 mag/arcsec^2), have only been discovered in the Local Group. These galaxies are very low in mass (tens of 10^5 Msun) and compact (effective radius <1 kpc). These objects populate the least massive dark matter haloes capable of producing stars, providing us with valuable insights into the nature of star formation at
    Montes, Mireia

    Fecha de publicación:

    7
    2024
    Número de citas
    0
  • An extended low-density atmosphere around the Jupiter-sized planet WASP-193 b
    Gas giants transiting bright nearby stars provide crucial insights into planetary system formation and evolution mechanisms. Most of these planets show certain average characteristics, serving as benchmarks for our understanding of planetary systems. However, outliers like the planet we present in this study, WASP-193 b, offer unique opportunities
    Barkaoui, Khalid et al.

    Fecha de publicación:

    7
    2024
    Número de citas
    6
  • Age of Massive Galaxies at Redshift 8
    Recent James Webb Space Telescope data analyses have shown that massive red galaxies existed at redshifts z ≳ 6, a discovery that is difficult to understand in the context of standard cosmology (ΛCDM). Here, we analyze these observations more deeply, by fitting a stellar population model to the optical and near-infrared photometric data. These fits
    López-Corredoira, M. et al.

    Fecha de publicación:

    7
    2024
    Número de citas
    6
  • Active optics control and its integration with the adaptive optics in the European Solar Telescope (EST)
    The European Solar Telescope (EST) is a 4-m class solar telescope that will include a Multiconjugate Adaptive Optics system (MCAO) integrated in the telescope optical path. Its open-dome configuration implies that the complete telescope will be exposed to wind, having an important impact in image stability and quality. The integration of Active
    León-Gil, J. et al.

    Fecha de publicación:

    7
    2024
    Número de citas
    0
  • Accretion-induced variability of interacting red giant binaries masquerading as oscillations
    Symbiotic stars are strongly interacting binaries with long orbital periods, containing an evolved red giant and a white dwarf or a neutron star embedded in a circumbinary nebula. They constitute unique astrophysical laboratories important for understanding the binary evolution and diverse processes occurring also in many other types of
    Merc, Jaroslav et al.

    Fecha de publicación:

    7
    2024
    Número de citas
    0