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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  • Brown dwarfs and very low mass stars in the Praesepe open cluster: a dynamically unevolved mass function?
    Context. Determination of the mass functions of open clusters of different ages allows us to infer the efficiency with which brown dwarfs are evaporated from clusters to populate the field. Aims: In this paper we present the results of a photometric survey to identify low mass and brown dwarf members of the old open cluster Praesepe (age 590+150
    Boudreault, S. et al.

    Fecha de publicación:

    2
    2010
    Número de citas
    28
  • Apparent Novae in M81: M81N 2010-01a and M81N 2010-01b
    CBET 2170 available at Central Bureau for Astronomical Telegrams.
    Hornoch, K. et al.

    Fecha de publicación:

    2
    2010
    Número de citas
    0
  • Apparent Novae in M81: M81N 2010-01a and M81N 2010-01b
    CBET 2170 available at Central Bureau for Astronomical Telegrams.
    Hornoch, K. et al.

    Fecha de publicación:

    2
    2010
    Número de citas
    1
  • Apparent Nova in M81: M81N 2010-01c
    CBET 2180 available at Central Bureau for Astronomical Telegrams.
    Hornoch, K. et al.

    Fecha de publicación:

    2
    2010
    Número de citas
    0
  • An HST/WFPC2 survey of bright young clusters in M 31. IV. Age and mass estimates
    Aims: We present the main results of an imaging survey of possible young massive clusters (YMC) in M 31 performed with the Wide Field and Planetary Camera 2 (WFPC2) on the Hubble Space Telescope (HST), with the aim of estimating their age and their mass. We obtained shallow (to B ˜ 25) photometry of individual stars in 19 clusters (of the 20
    Perina, S. et al.

    Fecha de publicación:

    2
    2010
    Número de citas
    28
  • A scenario of planet erosion by coronal radiation
    Context. According to theory, high-energy emission from the coronae of cool stars can severely erode the atmospheres of orbiting planets. No observational tests of the long-term erosion effects have been made yet. Aims: We analyze the current distribution of planetary mass with X-ray irradiation of the atmospheres to make an observational
    Sanz-Forcada, J. et al.

    Fecha de publicación:

    2
    2010
    Número de citas
    74