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 Study of Post-Agb Stars in the Light of GAIA DR3 Data
    Low and intermediate-mass stars evolve through the Post Asymptotic Giant Branch (post-AGB) phase before they reach the Planetary Nebulae stage. After leaving the Main Sequence, they undergo intense episodes of mass loss when in the Giant Branch and, then, they enter the post-AGB stage which is a rather puzzling stellar evolutionary phase . Also, it
    Manteiga, Minia et al.

    Fecha de publicación:

    8
    2024
    Número de citas
    0
  • A search for Galactic post-asymptotic giant branch stars in Gaia DR3
    Context. When low- and intermediate-mass stars leave the asymptotic giant branch (AGB) phase, and before they reach the planetary nebula stage, they enter a very brief and rather puzzling stellar evolutionary stage called post-AGB stage. The post-AGB phase lasts very briefly, about a few thousand years at most. The number of objects that are
    González-Santamaría, I. et al.

    Fecha de publicación:

    8
    2024
    Número de citas
    0
  • A low-mass sub-Neptune planet transiting the bright active star HD 73344
    Context. Planets with radii of between 2 and 4 R ⊕ closely orbiting solar-type stars are of significant importance for studying the transition from rocky to giant planets, and are prime targets for atmospheric characterization by missions such as JWST and ARIEL. Unfortunately, only a handful of examples with precise mass measurements are known to
    Sulis, S. et al.

    Fecha de publicación:

    8
    2024
    Número de citas
    1
  • A hot-Jupiter progenitor on a super-eccentric retrograde orbit
    Giant exoplanets orbiting close to their host stars are unlikely to have formed in their present configurations 1. These `hot Jupiter' planets are instead thought to have migrated inward from beyond the ice line and several viable migration channels have been proposed, including eccentricity excitation through angular-momentum exchange with a third
    Gupta, Arvind F. et al.

    Fecha de publicación:

    8
    2024
    Número de citas
    8
  • A benchmark JWST near-infrared spectrum for the exoplanet WASP-39 b
    Observing exoplanets through transmission spectroscopy supplies detailed information about their atmospheric composition, physics and chemistry. Before the James Webb Space Telescope (JWST), these observations were limited to a narrow wavelength range across the near-ultraviolet to near-infrared, alongside broadband photometry at longer wavelengths
    Carter, A. L. et al.

    Fecha de publicación:

    8
    2024
    Número de citas
    12
  • [Mg/Fe] and variable initial mass function: Revision of [α/Fe] for massive galaxies
    Observations of nearby massive galaxies have revealed that they are older and richer in metals and magnesium than their low-mass counterparts. In particular, the overabundance of magnesium compared to iron, [Mg/Fe], is interpreted to reflect the short star formation history that the current massive galaxies underwent early in the Universe. We
    Pernet, Emilie et al.

    Fecha de publicación:

    7
    2024
    Número de citas
    5