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

  • A high fraction of close massive binary stars at low metallicity
    At high metallicity, a majority of massive stars have at least one close stellar companion. The evolution of such binaries is subject to strong interaction processes, which heavily impact the characteristics of their life-ending supernova and compact remnants. For the low-metallicity environments of high-redshift galaxies, constraints on the
    Sana, H. et al.

    Fecha de publicación:

    9
    2025
    Número de citas
    2
  • A Descriptive Taxonomic Nomenclature for Intermediate-sized Trans-Neptunian Object Spectra
    Trans-Neptunian objects (TNOs), icy remnants of planet formation orbiting beyond Neptune, comprise a dynamically and compositionally diverse population of >5000 known members. An extensive body of literature focuses on the dynamical structure of the trans-Neptunian region. Less information is available on TNO compositions due to the difficulty
    Holler, Bryan J. et al.

    Fecha de publicación:

    9
    2025
    Número de citas
    0
  • (163) Erigone, (302) Clarissa, and (752) Sulamitis as seen with JWST's NIRSpec
    Primitive asteroids in the Main Belt possess one of the most pristine inventories of materials in the Solar System. Main Belt primitive asteroids are particularly interesting due to clear evidence of phyllosilicates, i.e., silicates that have encountered liquid water and undergone chemical alteration. Since asteroids are thought to be likely
    Harvison, Brittany et al.

    Fecha de publicación:

    9
    2025
    Número de citas
    0
  • Variable stars in Local Group galaxies: VII. New insights into the Leo II dSph
    Aims. Pulsating variable stars are invaluable tracers for reconstructing the star formation history and chemical evolution of their host galaxies. In this work, we explore the variable star population of Leo II, a distant dwarf spheroidal satellite of the Milky Way. Methods. We analyse an extensive dataset of ground-based BVRI time-series
    Monelli, M. et al.

    Fecha de publicación:

    8
    2025
    Número de citas
    0
  • TOI-1846 b: a super-Earth in the radius valley orbiting a nearby M dwarf
    We present the discovery and validation of a super-Earth planet orbiting the M dwarf star TOI-1846 (TIC 198385543). The host star ( $K_{\rm mag} = 9.6$) is located 47 pc away and has a radius of $R_\star = 0.41 \pm 0.01$ $\rm \, R_\odot$, a mass of $M_\star = 0.40 \pm 0.02$ $\rm \, M_\odot$ and an effective temperature of $T_{\rm eff} = 3568 \pm 44
    Soubkiou, Abderahmane et al.

    Fecha de publicación:

    8
    2025
    Número de citas
    0
  • Tidal Debris Candidates from the ω Centauri Accretion Event and Its Role Building Up the Milky Way Halo
    We identify stellar tidal debris from the ω Centauri (ω Cen) system among field stars in the Apache Point Observatory Galactic Evolution Experiment (APOGEE) survey via chemical tagging using a neural network trained on APOGEE observations of the ω Cen core. We find a total of 463 ω Cen debris candidates have a probability P > 0.8 of sharing common
    Anguiano, Borja et al.

    Fecha de publicación:

    8
    2025
    Número de citas
    2