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

  • Asteroid sizes determined with thermophysical model and stellar occultations
    Context. The sizes of many asteroids, especially slowly rotating, low-amplitude targets, remain poorly constrained due to selection effects. These biases limit the availability of high-quality data, leaving size estimates reliant on spherical shape assumptions. Such approximations introduce significant uncertainties propagating, for example, into
    Choukroun, A. et al.

    Fecha de publicación:

    6
    2025
    Número de citas
    0
  • ASASSN–14dx: a cataclysmic variable harbouring a massive pulsating white dwarf
    We present the results of our study of ASASSN–14dx, a previously known but poorly characterized cataclysmic variable (CV). The source was observed as part of an ongoing high-time-resolution photometric survey of CVs, which revealed that, in addition to the known 82.8-min orbital period, it also exhibits other transient periods, the strongest of
    Hakala, Pasi et al.

    Fecha de publicación:

    6
    2025
    Número de citas
    0
  • Analysis of optical spectroscopy and photometry of the type I X-ray bursting system UW CrB
    UW Coronae Borealis (UW CrB) is a low mass X-ray binary that shows both Type 1 X-ray and optical bursts, which typically last for 20 s. The system has a binary period of close to 2 hours and is thought to have a relatively high inclination due to the presence of an eclipse in the optical light curve. There is also evidence that an asymmetric disc
    Kennedy, Mark R. et al.

    Fecha de publicación:

    6
    2025
    Número de citas
    0
  • Accretion Diagnostics for JWST–MIRI: Establishing the Relationship between Mid-Infrared Hydrogen Lines and the Accretion Luminosity
    We have established mid-infrared hydrogen recombination lines observed with JWST as accretion tracers for pre-main-sequence stars that accrete from circumstellar disks. These new relations equip the community with a direct measurement of the accretion luminosity from MIRI-MRS spectra. A MIRI-derived accretion luminosity is fundamental for time
    Tofflemire, Benjamin et al.

    Fecha de publicación:

    6
    2025
    Número de citas
    0
  • A transiting rocky super-Earth and a non-transiting sub-Neptune orbiting the M dwarf TOI-771
    Context. The origin and evolution of the sub-Neptune population is a highly debated topic in the exoplanet community. With the advent of JWST, atmospheric studies can now put unprecedented constraints on the internal composition of this population. In this context, the THIRSTEE project aims to investigate the population properties of sub-Neptunes
    Lacedelli, G. et al.

    Fecha de publicación:

    6
    2025
    Número de citas
    0
  • A transiting multiplanet system in the 61 Myr old association Theia 116
    Observing and characterizing young planetary systems can aid in unveiling the evolutionary mechanisms that sculpt the mature exoplanet population. As an all-sky survey, NASA's Transiting Exoplanet Survey Satellite (TESS) has expanded the known young planet population as it has observed young comoving stellar populations. This work presents the
    Vach, Sydney et al.

    Fecha de publicación:

    6
    2025
    Número de citas
    2