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

  • Sin árbitro
    On the relation between the maximum stellar mass and the star cluster mass.
    Not Available
    Weidner, C. et al.

    Fecha de publicación:

    8
    2005
    Bibcode
    2005AN....326..605W
    Número de citas
    2
  • Con árbitro
    On the orientation of ancient Egyptian temples: (1) Upper Egypt and lower Nubia
    Not Available
    Shaltout, Mosalam et al.

    Fecha de publicación:

    8
    2005
    Bibcode
    2005JHA....36..273S
    Número de citas
    8
  • Con árbitro
    On the nature of lithium-rich giant stars. Constraints from beryllium abundances
    We have derived beryllium abundances for 7 Li-rich giant (A(Li) > 1.5) stars and 10 other Li-normal giants with the aim of investigating the origin of the lithium in the Li-rich giants. In particular, we test the predictions of the engulfment scenario proposed by Siess & Livio (1999, MNRAS, 308, 1133), where the engulfment of a brown dwarf or one
    Melo, C. H. F. et al.

    Fecha de publicación:

    8
    2005
    Bibcode
    2005A&A...439..227M
    Número de citas
    33
  • Sin árbitro
    Near-infrared Spectra of Two Asteroids with Low Tisserand Invariant
    We present near-infrared reflectance spectra of two asteroids with low Tisserand invariant, 2906 Caltech and 1373 Cincinnati. The Tisserand invariant is a commonly used dynamical discriminator, with values less than 3 considered suggestive of cometary origin. Asteroids Caltech and Cincinnati have Tisserand invariant values of 2.97 and 2.72
    Ziffer, J. et al.

    Fecha de publicación:

    8
    2005
    Bibcode
    2005DPS....37.1529Z
    Número de citas
    0
  • Sin árbitro
    Jupiter Trojans: a Survey of Members of Dynamical Families
    Since 2002, we started an observational program on Jupiter Trojans at ESO-NTT, ESO-VLT and TNG. We carried out visible and near-infrared spectroscopy and photometry of members of dynamical families, as defined by Beauge and Roig (2001), and of several background objects. The aim of these observations was to improve our knowledge of the surface
    Dotto, E. et al.

    Fecha de publicación:

    8
    2005
    Bibcode
    2005DPS....37.0305D
    Número de citas
    0