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

  • On the origin of the ultramassive white dwarf GD50
    We argue on the basis of astrometric and spectroscopic data that the ultramassive white dwarf GD50 is associated with the star formation event that created the Pleiades and is possibly a former member of this cluster. Its cooling age (~60 Myr) is consistent with it having evolved essentially as a single star from a progenitor with a mass M >
    Dobbie, P. D. et al.

    Fecha de publicación:

    11
    2006
    Número de citas
    40
  • On the Connection Between Solar Activity and Low-Latitude Aurorae in the Period 1715 - 1860
    Observations of aurorae borealis at low latitudes are very rare and are clearly associated with strong geomagnetic storms. Morphologically, they are characterized by a diffuse red colour with no rapid motions. The main aim of this paper is to analyse two hitherto ignored aurorae that were observed at two low-latitude sites, Tenerife (28°N 18°W) and
    Vázquez, M. et al.

    Fecha de publicación:

    11
    2006
    Número de citas
    18
  • New Times of Minima of Some Eclipsing Binary Systems
    We present 42 photoelectric minima observations of 24 eclipsing binaries.
    Csizmadia, Sz. et al.

    Fecha de publicación:

    11
    2006
    Número de citas
    14
  • New members in the Upper Scorpius association from the UKIRT Infrared Deep Sky Survey Early Data Release†
    We present the results of a 9.3-deg2 infrared (ZYJHK) survey in the Upper Scorpius association extracted from the UKIRT Infrared Deep Sky Survey (UKIDSS) Galactic Cluster Survey Early Data Release. We have selected a total of 112 candidates from the (Z - J,Z) colour-magnitude diagram over the Z = 12.5-20.5 magnitude range, corresponding to M = 0.25
    Lodieu, N. et al.

    Fecha de publicación:

    11
    2006
    Número de citas
    48
  • Near-IR variability properties of a selected sample of AGB stars
    We present the results of a near-infrared monitoring programme of a selected sample of stars, initially suspected to be Mira variables and OH/IR stars, covering more than a decade of observations. The objects monitored cover the typical range of IRAS colours shown by O-rich stars on the asymptotic giant branch and show a surprisingly large
    Jiménez-Esteban, F. M. et al.

    Fecha de publicación:

    11
    2006
    Número de citas
    15