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

  • Rol de la transferencia de masa en binarias de objetos compactos
    Understanding the properties, formation, and evolutionary path of high- mass star systems is a fundamental research topic in stellar astrophysics. Under certain conditions, massive binaries form gravitationally bound compact objects capable of merging in less than the age of the Universe, producing gravitational waves detectable by observatories
    Astudillo, J. et al.

    Fecha de publicación:

    8
    2025
    Número de citas
    0
  • Roadmap on carbon molecular nanostructures in space
    In this roadmap article, we consider the main challenges and recent breakthroughs in understanding the role of carbon molecular nanostructures in space and propose future avenues of research. The focus lies on small carbon-containing molecules up to fullerenes, extending to even larger, more complex organic species. The roadmap contains forty
    Hansen, Klavs et al.

    Fecha de publicación:

    8
    2025
    Número de citas
    0
  • Revisiting the hypothesis of purely stochastic excitation of global p modes in the Sun
    Context. In solar-like oscillators, acoustic waves are excited by turbulent motion in the convective envelope and propagate inward, generating a variety of standing pressure modes (p modes). When combining the power of several solar acoustic modes, some studies have reported an excess that is not compatible with pure stochastic excitation. This
    Panetier, E. et al.

    Fecha de publicación:

    8
    2025
    Número de citas
    0
  • Red supergiant stars in binary systems: II. Confirmation of B-type companions of red supergiants in the Small Magellanic Cloud using Hubble ultraviolet spectroscopy
    Red supergiant (RSG) stars represent the final evolutionary phase of the majority of massive stars and hold a unique role in testing the physics of stellar models. Eighty-eight RSGs in the Small Magellanic Cloud (SMC) were recently found to have an ultraviolet (UV) excess, which was attributed to a B-type companion. We present follow-up Hubble
    Patrick, L. R. et al.

    Fecha de publicación:

    8
    2025
    Número de citas
    5
  • Puzzling Variation of Gamma Rays from the Sun over the Solar Cycle Revealed with Fermi-LAT
    The steady-state gamma-ray emission from the Sun is thought to consist of two emission components due to interactions with Galactic cosmic rays: (1) a hadronic disk component, and (2) a leptonic extended component peaking at the solar edge and extending into the heliosphere. The flux of these components is expected to vary with the 11 yr solar
    Acharyya, A. et al.

    Fecha de publicación:

    8
    2025
    Número de citas
    3
  • Puzzling radial gradients of K-band absorption features in the giant elliptical galaxy M87
    We present new K-band spectroscopy for the giant elliptical galaxy M87 in the Virgo cluster, taken with the Large Binocular Telescope Utility Camera in the Infrared (LUCI) spectrograph at the Large Binocular Telescope (LBT). The new data are used to study line strengths of K-band absorption features from different chemical species, namely Fe, Mg
    La Barbera, F. et al.

    Fecha de publicación:

    8
    2025
    Número de citas
    0