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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  • WASP-14 b: transit timing analysis of 19 light curves
    Although WASP-14 b is one of the most massive and densest exoplanets on a tight and eccentric orbit, it has never been a target of photometric follow-up monitoring or dedicated observing campaigns. We report on new photometric transit observations of WASP-14 b obtained within the framework of Transit Timing Variations @ Young Exoplanet Transit
    Raetz, St. et al.

    Fecha de publicación:

    8
    2015
    Número de citas
    18
  • Thermophysical modeling of asteroids from WISE thermal infrared data - Significance of the shape model and the pole orientation uncertainties
    In the analysis of thermal infrared data of asteroids by means of thermophysical models (TPMs) it is a common practice to neglect the uncertainty of the shape model and the rotational state, which are taken as an input for the model. Here, we present a novel method of investigating the importance of the shape model and the pole orientation
    Hanuš, J. et al.

    Fecha de publicación:

    8
    2015
    Número de citas
    64
  • The VLT-FLAMES Tarantula Survey. XXII. Multiplicity properties of the B-type stars
    We investigate the multiplicity properties of 408 B-type stars observed in the 30 Doradus region of the Large Magellanic Cloud with multi-epoch spectroscopy from the VLT-FLAMES Tarantula Survey (VFTS). We use a cross-correlation method to estimate relative radial velocities from the helium and metal absorption lines for each of our targets. Objects
    Dunstall, P. R. et al.

    Fecha de publicación:

    8
    2015
    Número de citas
    156
  • The trace of a substantial assembly of massive E-S0 galaxies at 0.8 < z < 1.5 in galaxy number counts
    K-band galaxy number counts (GNCs) exhibit a slope change at K ˜ 17.5 mag not present in optical bands. To unveil the nature of this feature, we have derived the contribution of different galaxy types to the total K-band GNCs at 0.3 z 1.5 by redshift bins and compared the results with expectations from several galaxy evolutionary models. We show
    Prieto, M. et al.

    Fecha de publicación:

    8
    2015
    Número de citas
    7
  • The post-common envelope central stars of the planetary nebulae Henize 2-155 and Henize 2-161
    We present a study of Hen 2-155 and Hen 2-161, two planetary nebulae which bear striking morphological similarities to other planetary nebulae known to host close-binary central stars. Both central stars are revealed to be photometric variables while spectroscopic observations confirm that Hen 2-155 is host to a double-eclipsing, post-common
    Jones, D. et al.

    Fecha de publicación:

    8
    2015
    Número de citas
    60
  • The planetary nebulae in NGC6822 revisited
    Spectroscopic data for 20 PNe in the irregular galaxy NGC6822 have been studied. This represents 80% of the total sample of PNe candidates in this galaxy. We discuss the kinematics of PNe in comparison to the kinematics of the HI disk and the young and intermediate age populations. In addition the chemical abundances of the sample have been
    Pena, M. et al.

    Fecha de publicación:

    8
    2015
    Número de citas
    0