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..

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  • Two almost planetary mass survivors of common envelope evolution
    White dwarfs are often found in close binaries with stellar or even substellar companions. It is generally thought that these compact binaries form via common envelope evolution, triggered by the progenitor of the white dwarf expanding after it evolved off the main sequence and engulfing its companion. To date, a handful of white dwarfs in compact
    Parsons, S. G. et al.

    Fecha de publicación:

    2
    2025
    Número de citas
    0
  • Transit-timing variations in the AU Mic system observed with CHEOPS
    Context. AU Mic is a very active M dwarf star with an edge-on debris disk and two known transiting sub-Neptunes with a possible third planetary companion. The two transiting planets exhibit significant transit-timing variations (TTVs) that are caused by the gravi tational interaction between the bodies in the system. Aims. Using photometrical
    Boldog, Á. et al.

    Fecha de publicación:

    2
    2025
    Número de citas
    0
  • TOI-5108 b and TOI 5786 b: Two transiting sub-Saturns detected and characterized with TESS, MaHPS, and SOPHIE
    We report the discovery and characterization of two sub-Saturns from the Transiting Exoplanet Survey Satellite (TESS) using high- resolution spectroscopic observations from the MaHPS spectrograph at the Wendelstein Observatory and the SOPHIE spectrograph at the Haute-Provence Observatory. Combining photometry from TESS, KeplerCam, LCOGT, and
    Thomas, Luis et al.

    Fecha de publicación:

    2
    2025
    Número de citas
    0
  • Titanium chemistry of WASP-121 b with ESPRESSO in 4-UT mode
    Transit spectroscopy usually relies on the integration of one or several transits to achieve the signal-to-noise ratio (S/N) necessary to resolve spectral features. Consequently, high-S/N observations of exoplanet atmospheres, where we can forgo integration, are essential for disentangling the complex chemistry and dynamics beyond global trends. In
    Prinoth, B. et al.

    Fecha de publicación:

    2
    2025
    Número de citas
    0
  • Time-dependent modelling of short-term variability in the TeV-blazar VER J0521+211 during the major flare in 2020
    The BL Lacertae object VER J0521+211 underwent a notable flaring episode in February 2020. A short-term monitoring campaign, led by the MAGIC (Major Atmospheric Gamma Imaging Cherenkov) collaboration, covering a wide energy range from radio to very high-energy (VHE, 100 GeV < E < 100 TeV) gamma rays was organised to study its evolution. These
    MAGIC Collaboration et al.

    Fecha de publicación:

    2
    2025
    Número de citas
    0
  • Thermal evolution of trans-Neptunian objects through observations of Centaurs with JWST
    Centaurs are small bodies orbiting between Jupiter and Neptune and behave as an intermediate population between trans-Neptunian-belt objects and Jupiter-family comets. As such, their surface composition and evolutionary processes are key to understanding the Solar System's history. However, the mechanisms driving their transformation and the impact
    Licandro, Javier et al.

    Fecha de publicación:

    2
    2025
    Número de citas
    2