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

  • Evolution of the Star Formation Rate at z ~ 0.2 and z ~ 0.4 from Hα
    Not Available
    Pascual, S. et al.

    Fecha de publicación:

    0
    2001
    Número de citas
    0
  • Evidence of a Supernova Origin for the Black Hole in GRO J1655-40 (Nova Scorpii 1994)
    We report the discovery of a strong overabundance of several α-elements in the atmosphere of the star orbiting around the massive black hole in the binary system GRO J1655-40 (Nova Scorpii 1994). A high-resolution spectrum of this star obtained with the Keck I 10m telescope reveals the presence of extra strong absorption lines of O, Mg, Si, and S
    Israelian, Garik

    Fecha de publicación:

    0
    2001
    Número de citas
    0
  • Evidence for Free-floating Planetary-mass Objects in the σ Orionis Star Cluster (CD-ROM Directory: contribs/osorio)
    Not Available
    Zapatero Osorio, M. R. et al.

    Fecha de publicación:

    0
    2001
    Número de citas
    1
  • Euro50: Proposal for a 50 m Optical and Infrared Telescope
    Staff from Instituto de Astrofisica de Canarias, Lund Observatory, Physics Department and Larmor Research Institute at Galway, and Tuorla Observatory is collaborating on studies for a 50 m optical and infrared telescope. The telescope concepts are based on the work on extremely large telescopes carried out during 1991-2000 at Lund Observatory, and
    Ardeberg, Arne et al.

    Fecha de publicación:

    0
    2001
    Número de citas
    0
  • Double Bars, Inner Disks, and Nuclear Rings in Barred Galaxies
    We present results of a high-resolution imaging survey of barred S0--Sa galaxies which demonstrate that the central regions of these galaxies are surprisingly complex. We see many inner bars---small, secondary bars (typically less than a kiloparsec in radius) located inside of, and probably rotating faster than, the large primary bars. These are
    Erwin, Peter et al.

    Fecha de publicación:

    0
    2001
    Número de citas
    6