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

  • Sub-Neptune Atmospheres at High Resolution with ANDES: Can We Observe Robust Signals?
    The most probable outcome of planetary formation is a sub-Neptune, a body with a radius between 2.0 and 3.5 Earth radii. This type of exoplanet has no counterpart in the Solar System, but they are very common elsewhere, and many of them have been observed to potentially host habitable surface conditions. Population studies have revealed a scarcity
    Peáez-Torres, A. et al.

    Fecha de publicación:

    5
    2025
    Número de citas
    0
  • Structure and Dynamics of the Sun's Interior Revealed by the Helioseismic and Magnetic Imager
    High-resolution helioseismology observations with the Helioseismic and Magnetic Imager (HMI) onboard the Solar Dynamics Observatory (SDO) provide a unique three-dimensional view of the solar interior structure and dynamics, revealing a tremendous complexity of the physical processes inside the Sun. We present an overview of the results of the HMI
    Kosovichev, Alexander G. et al.

    Fecha de publicación:

    5
    2025
    Número de citas
    0
  • Spatially-resolved stellar population properties of galaxies in voids with the CAVITY project
    Galaxies in voids have been found to be of a later type, bluer, less massive, and to have a slower evolution than galaxies in denser environments (filaments and walls). However, the effect of the void environment on their stellar population properties is still unclear. We aim to address this question using 118 optical integral field unit datacubes
    Conrado, A. et al.

    Fecha de publicación:

    5
    2025
    Número de citas
    0
  • Size and shape of the trans-Neptunian object (470316) 2007 OC10: Comparison with thermal data
    Context. The shapes of only 12 trans-Neptunian objects have been directly measured, offering crucial insights into their internal structure. These properties are strongly connected to the processes that shaped the early Solar System, and provide important clues about its evolution. Aims. The aim of the present work is to characterise the size
    Gómez-Limón, J. M. et al.

    Fecha de publicación:

    5
    2025
    Número de citas
    0
  • Signature of spin-down stalling in stellar magnetic activity: The case of the open cluster NGC 6811
    Context. Stellar rotation and magnetic activity have a complex evolution that reveals multiple regimes. One of the related transitions that is seen in the rotation distribution for main-sequence (MS) solar-like stars has been attributed to core-envelope coupling and the consequent angular-momentum transfer between a fast core and a slow envelope
    Santos, A. R. G. et al.

    Fecha de publicación:

    5
    2025
    Número de citas
    1
  • Searching for R-process-enhanced Stars in the LAMOST Survey. II. Two New r-II Stars in the Milky Way Disk
    R-process-enhanced (RPE) stars are rare and typically metal-poor ([Fe/H] < ‑1.0), primarily found in the Milky Way halo system and dwarf galaxies. This study reports the discovery of two relatively bright, highly RPE stars ([Eu/Fe] > +0.70) located in the Milky Way disk, with [Fe/H] of ‑0.34 and ‑0.80, respectively. These two stars are selected
    Xie, Xiao-Jin et al.

    Fecha de publicación:

    5
    2025
    Número de citas
    0