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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  • K2-139 b: a low-mass warm Jupiter on a 29-d orbit transiting an active K0 V star
    We announce the discovery of K2-139 b (EPIC 218916923 b), a transiting warm-Jupiter (Teq = 547 ± 25 K) on a 29-d orbit around an active (log R^' _HK = -4.46 ± 0.06) K0 V star in K2 Campaign 7. We derive the system's parameters by combining the K2 photometry with ground-based follow-up observations. With a mass of 0.387 _{ - 0.075 } ^ {+ 0.083 }MJ
    Barragán, O. et al.

    Fecha de publicación:

    4
    2018
    Número de citas
    20
  • Gas and dust from solar metallicity AGB stars
    We study the asymptotic giant branch (AGB) evolution of stars with masses between 1 M⊙and8.5 M⊙. We focus on stars with a solar chemical composition, which allows us to interpret evolved stars in the Galaxy. We present a detailed comparison with models of the same chemistry, calculated with a different evolution code and based on a different set of
    Ventura, P. et al.

    Fecha de publicación:

    4
    2018
    Número de citas
    81
  • Frequency dependence of p-mode frequency shifts induced by magnetic activity in Kepler solar-like stars
    The variations of the frequencies of the low-degree acoustic oscillations in the Sun induced by magnetic activity show a dependence on radial order. The frequency shifts are observed to increase towards higher-order modes to reach a maximum of about 0.8 μHz over the 11-yr solar cycle. A comparable frequency dependence is also measured in two other
    García, R. A. et al.

    Fecha de publicación:

    4
    2018
    Número de citas
    31
  • First Observation of the Submillimeter Polarization Spectrum in a Translucent Molecular Cloud
    Polarized emission from aligned dust is a crucial tool for studies of magnetism in the ISM, but a troublesome contaminant for studies of cosmic microwave background polarization. In each case, an understanding of the significance of the polarization signal requires well-calibrated physical models of dust grains. Despite decades of progress in
    Ashton, P. C. et al.

    Fecha de publicación:

    4
    2018
    Número de citas
    39
  • Extreme magnification of an individual star at redshift 1.5 by a galaxy-cluster lens
    Galaxy-cluster gravitational lenses can magnify background galaxies by a total factor of up to 50. Here we report an image of an individual star at redshift z = 1.49 (dubbed MACS J1149 Lensed Star 1) magnified by more than ×2,000. A separate image, detected briefly 0.26″ from Lensed Star 1, is probably a counterimage of the first star demagnified
    Kelly, Patrick L. et al.

    Fecha de publicación:

    4
    2018
    Número de citas
    165
  • Extended X-ray emission in PKS 1718-649
    PKS 1718-649 is one of the closest and most comprehensively studied candidates of a young active galactic nucleus (AGN) that is still embedded in its optical host galaxy. The compact radio structure, with a maximal extent of a few parsecs, makes it a member of the group of compact symmetric objects (CSO). Its environment imposes a turnover of the
    Beuchert, T. et al.

    Fecha de publicación:

    4
    2018
    Número de citas
    18