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

  • HS 0943+1404, a true intermediate polar
    We have identified a new intermediate polar, HS 0943+1404, as part of our ongoing search for cataclysmic variables in the Hamburg Quasar Survey. The orbital and white dwarf spin periods determined from time-resolved photometry and spectroscopy are Porb ≃ 250 min and Pspin= 69.171 ± 0.001 min, respectively. The combination of a large ratio Pspin
    Rodríguez-Gil, P. et al.

    Fecha de publicación:

    9
    2005
    Número de citas
    17
  • HST Astrometry in the 30 Doradus Region. II. Runaway Stars from New Proper Motions in the Large Magellanic Cloud
    We present a catalog of relative proper motions for 368,787 stars in the 30 Doradus region of the Large Magellanic Cloud (LMC), based on a dedicated two-epoch survey with the Hubble Space Telescope and supplemented with proper motions from our pilot archival study. We demonstrate that a relatively short epoch difference of three years is sufficient
    Platais, I. et al.

    Fecha de publicación:

    9
    2018
    Número de citas
    16
  • Hubble Space Telescope and Ground-based Observations of V455 Andromedae Post-outburst
    Hubble Space Telescope spectra obtained in 2010 and 2011, 3 and 4 yr after the large amplitude dwarf nova outburst of V455 And, were combined with optical photometry and spectra to study the cooling of the white dwarf, its spin, and possible pulsation periods after the outburst. The modeling of the ultraviolet (UV) spectra shows that the white
    Szkody, Paula et al.

    Fecha de publicación:

    9
    2013
    Número de citas
    18
  • Hubble Space Telescope and Ground-based Spectroscopy of K648 in M15
    We derive some element abundances for the central star of the planetary nebula K648 from analysis of Hubble Space Telescope Faint Object Spectrograph spectra (1200-3300 Å). Carbon is found to be approximately 4 times overabundant with respect to solar values, while oxygen is underabundant and silicon about solar, and He/H=0.6. The stellar continuum
    Bianchi, Luciana et al.

    Fecha de publicación:

    9
    2001
    Número de citas
    24
  • HVC's Favouring Star Forming Processes in galaxy discs: a basic calculation and some recent HI observations
    Indirect evidence from detailed chemical evolution studies shows that infall of low metallicity gas appears to have proceeded at a rather constant rate during the lifetime of the Galactic disk. We explore two possible implications: (a) the effect of an infalling high velocity cloud (HVC) on interstellar cloud stability leading to enhanced star
    Buenrostro, V. et al.

    Fecha de publicación:

    9
    2012
    Número de citas
    0
  • IAC-STAR: A Code for Synthetic Color-Magnitude Diagram Computation
    The code IAC-STAR is presented. It generates synthetic H-R and color-magnitude diagrams (CMDs) and is mainly aimed at star formation history studies in nearby galaxies. Composite stellar populations are calculated on a star-by-star basis, by computing the luminosity, effective temperature, and gravity of each star by direct bilogarithmic
    Aparicio, Antonio et al.

    Fecha de publicación:

    9
    2004
    Número de citas
    157