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 hard ultraluminous state of NGC 5055 ULX X-1
    We present the results of the first broadband X-ray analysis of the ultraluminous X-ray source NGC 5055 ULX X-1, combining simultaneous data from XMM─Newton and NuSTAR missions, with a combined exposure time of ∼100 ks across the 0.3─20 keV energy range. The source exhibits a stable flux across the entire exposure with no detectable pulsations by
    Cruz-Sanchez, N. et al.

    Fecha de publicación:

    1
    2026
    Número de citas
    0
  • The Galaxy Activity, Torus, and Outflow Survey (GATOS): X. Molecular gas clumpiness under the influence of AGN
    The distribution of molecular gas on small scales regulates star formation and the growth of supermassive black holes in galaxy centers. Yet, the role of active galactic nuclei (AGN) feedback in shaping this distribution remains poorly constrained. We investigate how AGNs influence the small-scale structure of molecular gas in galaxy centers by
    Esposito, Federico et al.

    Fecha de publicación:

    1
    2026
    Número de citas
    0
  • TESS Investigation—Demographics of Young Exoplanets (TI-DYE). IV. A Jovian-radius Planet Orbiting a 34 Myr Sun-like Star in the Vela Association
    The discovery of infant (<50 Myr), close-in (<30-day-period) planets is vital in understanding the formation mechanisms that lead to the distribution of mature transiting planets as discovered by Kepler. Despite several discoveries in this age bin, the sample is still too small for a robust statistical comparison to older planets. Here we report
    Barber, Madyson G. et al.

    Fecha de publicación:

    1
    2026
    Número de citas
    0
  • Supernova Ia Remnants with M-dwarf Surviving Companions
    We study the possibility that Type Ia supernovae might be produced by binary systems where the companion of the exploding white dwarf is an M-dwarf star. Such a companion would appear as a runaway star, retaining its pre-explosion orbital velocity along with a kick imparted by the supernova ejecta. It might be rapidly rotating, from being tidally
    Pan, Kuo-Chuan et al.

    Fecha de publicación:

    1
    2026
    Número de citas
    3
  • Stellar populations in satellite galaxies in close pairs
    Satellite galaxies that are near to massive primary galaxies in close pairs can have stellar population ages that are more similar to their primaries than expected. This is one way in which close pairs of galaxies show galactic conformity, which is thought to be driven by assembly bias. Such conformity is seen in ages, morphologies, and star
    Sansom, A. E. et al.

    Fecha de publicación:

    1
    2026
    Número de citas
    0
  • Spin Parameters and Shape Models of Near-Earth Asteroids (4660) Nereus, (21088) Chelyabinsk, (66146) 1998 TU3, and (297418) 2000 SP43
    We present our shape and rotational characterization of four near-Earth asteroids observed as part of the Visible NEAs Observations Survey. This work includes 61 new light curves obtained between 2020 June and 2024 September for asteroids (21088) Chelyabinsk and (66146) 1998 TU3 and the potentially hazardous asteroids (4660) Nereus and (297418)
    Rodríguez Rodríguez, Javier et al.

    Fecha de publicación:

    1
    2026