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

  • Symbiotic binaries in the Gaia data - II. Symbiotic candidates from general variability classification in DR3
    We investigate the reliability of the symbiotic star class in the general variability classification of Gaia Data Release 3 (DR3) and search for new genuine symbiotic systems among the objects assigned to this category. The sample contains 649 sources, including 246 previously known symbiotic stars, 61 literature candidates, and 339 new candidates
    Merc, J. et al.

    Fecha de publicación:

    9
    2026
    Número de citas
    0
  • Superorbital variability in the quiescent black hole X-ray transient A0620-00
    Quiescent black hole low-mass X-ray binaries provide a key setting for probing accretion physics at low luminosities. A0620--00, the archetypal system in this class, has remained in X-ray quiescence for decades and exhibits complex optical variability, yet the long-term behaviour of its accretion flow remains poorly understood. Here, we report an
    Saavedra, Enzo A. et al.

    Fecha de publicación:

    9
    2026
    Número de citas
    0
  • Star Cluster Populations in 38 Spiral Galaxies: Evidence for Near-universal Mass and Age Distributions from PHANGS
    We present the largest study to date of star cluster mass and age distributions in nearby galaxies. The analysis is based on a uniformly selected catalog of over 15,000 (36,000) human- (machine-) classified compact clusters across 38 spiral galaxies in the PHANGS-Hubble Space Telescope survey, with improved photometric SED age dating that mitigates
    Chandar, Rupali et al.

    Fecha de publicación:

    9
    2026
    Número de citas
    2
  • SPECFANN: Spectral Fitting via Artificial Neural Networks: I. A deep-learning-based FASTWIND emulator and fitting suite
    Context. The importance of massive stars cannot be overstated: they are powerful probes of the early universe, they play a vital role in the chemical and mechanical evolution of their host environments, and their end products allow us to study the most extreme physics in the universe. Obtaining accurate stellar and surface parameters for large
    Abdul-Masih, M. et al.

    Fecha de publicación:

    9
    2026
    Número de citas
    0
  • Spatial variations in polarized synchrotron emission in the QUIJOTE MFI data using neural networks
    Polarized synchrotron emission from ultra-relativistic electrons spiraling the Galactic magnetic field has recently become one of the most relevant emissions in the interstellar medium because the quality of low-frequency observations has improved. One recent experiment designed to explore this emission is QUIJOTE. We study the spatial variations
    Casas, J. M. et al.

    Fecha de publicación:

    9
    2026
    Número de citas
    1
  • Spatial correlations of PAH, UV, Hα emission and IMF─PAH variations in the star-forming complexes of NGC 628
    We examine the spatial correlation of emission from polycyclic aromatic hydrocarbons (PAH) (3.3, 7.7, and 11.3 $\mathrm{\mu m}$) with the far-ultraviolet (FUV), near-ultraviolet (NUV), and H $\alpha$ emission from star-forming complexes (SFCs) in different regions of NGC 628. We use the James Webb Space Telescope to detect PAH emission, along with
    Amrutha, S. et al.

    Fecha de publicación:

    9
    2026
    Número de citas
    0