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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  • Con árbitro
    Chemical Abundances of the Galactic H II Region NGC 3576 Derived from Very Large Telescope Echelle Spectrophotometry
    We present echelle spectrophotometry of the Galactic H II region NGC 3576. The data have been taken with the VLT UVES echelle spectrograph in the 3100-10400 Å range. We have measured the intensities of 458 emission lines, 344 are permitted lines of H0, He0, C+, N0, N+, N++, O0, O+, Ne+, S++, Si0, Si+, Ar0, and Ar+; some of them are produced by
    García-Rojas, Jorge et al.

    Fecha de publicación:

    8
    2004
    Bibcode
    2004ApJS..153..501G
    Número de citas
    106
  • Sin árbitro
    Book Review: Cosmochemistry. The melting pot of the elements / C. Esteban R. J. G. López, A. Herrero, F. Sánchez (eds.). Cambridge, Cambridge University Press, 2004, XII+298 pp., ISBN 0-521-82768-X
    Not Available
    Esteban, C. et al.

    Fecha de publicación:

    8
    2004
    Bibcode
    2004Orion..62U..37.
    Número de citas
    0
  • Sin árbitro
    Analysis of Simultaneous Visible and Infrared Spectropolarimetric Observations of Quiet Sun
    Not Available
    Domínguez Cerdeña, Itahiza et al.

    Fecha de publicación:

    8
    2004
    Bibcode
    2004ANS...325...94D
    Número de citas
    0
  • Sin árbitro
    a Relief to the Supersymmetric Fine Tuning Problem
    As is well known, electroweak breaking in the MSSM requires substantial fine-tuning. We explain why this fine tuning problem is abnormally acute, and this allows to envisage possible solutions to this undesirable situation. Following these ideas, we review some recent work which shows how in models with SUSY broken at a low scale (not far from the
    Casas, J. A. et al.

    Fecha de publicación:

    8
    2004
    Bibcode
    2004stph.conf...76C
    Número de citas
    15
  • Sin árbitro
    Using Globular Clusters to Test Newton's Law of Gravity
    New measurements of the velocity dispersion of the globular cluster ω Centauri allow us to trace its gravitational potential down to an acceleration of 8×10-9 cm s-2. It is found that the dispersion profile remains flat well inside the tidal radius as soon as the acceleration of gravity approaches a_0, a result that finds its simplest explanation
    Scarpa, R. et al.

    Fecha de publicación:

    7
    2004
    Bibcode
    2004IAUS..220..215S
    Número de citas
    9