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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  • Spectral characterization of near-Earth asteroids on cometary orbits
    A fraction of near-Earth asteroids has the orbital elements similar to those of comets, but a visual aspect as any other point-like source. These are potentially dormant comets nuclei who entered in a period of inactivity. Their study can provide a new understanding of the final state in which volatile-rich objects reside and of the existing
    Simion, Gabriel et al.

    Fecha de publicación:

    9
    2020
    Número de citas
    1
  • Single magnetic white dwarfs with Balmer emission lines: a small class with consistent physical characteristics as possible signposts for close-in planetary companions
    We report the identification of SDSS J121929.45+471522.8 as the third apparently isolated magnetic (B ≃ 18.5 ± 1.0 MG) white dwarf exhibiting Zeeman-split Balmer emission lines. The star shows coherent variability at optical wavelengths with an amplitude of ≃0.03 mag and a period of 15.26 h, which we interpret as the spin period of the white dwarf
    Gänsicke, Boris T. et al.

    Fecha de publicación:

    9
    2020
    Número de citas
    23
  • Search for Candidate Exogenous Material on Bennu using MapCam and PolyCam Images
    Introduction: Exogenous material has been reported on asteroids (101955) Bennu and (162173) Ryugu. The albedo, color, and spectra of six bright boulders on Bennu show that they are distinct from the rest of Bennu"s comparatively dark surface and are likely basaltic material from asteroid (4) Vesta (DellaGiustina et al. 2019; 2020). Bright boulders
    Campins, Humberto et al.

    Fecha de publicación:

    9
    2020
    Número de citas
    0
  • RoadRunner: a fast and flexible exoplanet transit model
    I present RoadRunner, a fast exoplanet transit model that can use any radially symmetric function to model stellar limb darkening (LD) while still being faster to evaluate than the analytical transit model for quadratic LD by Mandel & Agol. CPU and GPU implementations of the model are available in the PYTRANSIT transit modelling package, and come
    Parviainen, H.

    Fecha de publicación:

    9
    2020
    Número de citas
    10
  • Revisiting the atmosphere of HD 209458b with HARPS-N, CARMENES and ESPRESSO
    HD 209458b was the first transiting planet discovered, and the first for which its atmosphere, in particular Na I, was detected. With time, it has become one of the most studied planets, with a large diversity of atmospheric studies using low- and high-resolution spectroscopy. Here, we present the analysis of high-resolution transmission
    Casasayas-Barris, Núria et al.

    Fecha de publicación:

    9
    2020
    Número de citas
    0
  • Resonant absorption: Transformation of compressive motions into vortical motions
    This paper investigates the changes in spatial properties when magnetohydrodynamic (MHD) waves undergo resonant damping in the Alfvén continuum. The analysis is carried out for a 1D cylindrical pressure-less plasma with a straight magnetic field. The effect of the damping on the spatial wave variables is determined by using complex frequencies that
    Goossens, M. et al.

    Fecha de publicación:

    9
    2020
    Número de citas
    7