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

  • The impact of rotation on the stochastic excitation of stellar acoustic modes in solar-like pulsators
    Context. Recent observational results from asteroseismic studies show that an important fraction of solar-like stars do not present detectable stochastically excited acoustic oscillations. This non-detectability seems to correlate with a high rotation rate in the convective envelope and a high surface magnetic activity. At the same time, the
    Bessila, L. et al.

    Fecha de publicación:

    8
    2025
    Número de citas
    0
  • The Gondola for the SUNRISE III Balloon-Borne Solar Observatory
    SUNRISE III is a balloon-borne solar observatory dedicated to investigating the physics governing the magnetism and dynamics in the lower solar atmosphere. The observatory is designed to operate in the stratosphere, at heights around 36 km (above 99% of Earth's atmosphere), to avoid image degradation due to turbulence in the Earth's lower
    Bernasconi, Pietro et al.

    Fecha de publicación:

    8
    2025
    Número de citas
    0
  • The Gaia-ESO Survey: projected rotational velocities of B stars in the Carina Nebula
    The Carina Nebula is an active star-forming region with several open clusters rich in massive OB stars, thus making it an optimal target for studying stellar properties such as rotation for large samples of these early-type stars. We studied a sample of early-type stars probable members of the eight open clusters in the Carina Complex. The
    Santos, W. et al.

    Fecha de publicación:

    8
    2025
    Número de citas
    0
  • The ESPRESSO transmission spectrum of HD189733 b: Extracting the planetary sodium and lithium signatures amid stellar contamination
    Context. While transmission spectroscopy has allowed us to detect many atomic and molecular species in exoplanet atmospheres, the improvement in resolution and signal-to-noise ratio (S/N) enabled us to become sensitive to planet-occulted line distortions (POLDs) in the spectrum that are induced by center-to-limb variations (CLV) and the Rossiter
    Mounzer, D. et al.

    Fecha de publicación:

    8
    2025
    Número de citas
    0
  • The entropy of galaxy spectra
    The ability of any Machine Learning method to classify the spectra of galaxies depending on the properties of the stellar component rests on the information content of the data. The well-known degeneracies found in population synthesis models suggest this information might be so entangled as to challenge the most sophisticated Deep Learning
    Ferreras, I. et al.

    Fecha de publicación:

    8
    2025
    Número de citas
    0
  • The effect of local magnetic fields in quiet regions of stellar atmospheres simulated with MANCHA
    Context. In the past few years, new methods that allow measurement of local magnetic fields in photospheres of distant stars have been developed. The first simulations of a small-scale dynamo in stars other than the Sun have also been produced. While the nature of the small-scale fields is still under debate, it is an accepted fact that they can be
    Perdomo García, A. et al.

    Fecha de publicación:

    8
    2025
    Número de citas
    0