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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  • Deforming the Lie algebra of vector fields on $S^1$ inside the Poisson algebra on $dot T^*S^1$
    We study deformations of the standard embedding of the Lie algebra $Vect(S^1)$ of smooth vector fields on the circle, into the Lie algebra of functions on the cotangent bundle $T^*S^1$ (with respect to the Poisson bracket). We consider two analogous but different problems: (a) formal deformations of the standard embedding of $Vect(S^1)$ into the
    Ovsienko, V. et al.

    Fecha de publicación:

    7
    1997
    Número de citas
    0
  • Chemo-evolutionary Population Synthesis II. (Vazdekis+ 1997)
    We present the results of applying a new chemo-evolutionary stellar population model, developed in a previous paper, to new high-quality observational data of the nuclear regions of two representative elliptical galaxies and the bulge of the Sombrero galaxy. Here we fit in detail ~20 absorption lines and six optical and near-infrared colors
    Vazdekis, A. et al.

    Fecha de publicación:

    7
    1997
    Número de citas
    0
  • CCD photometry of the metal-rich halo cluster NGC 6366.
    We present new BV photometry for 6564 stars in the field of the globular cluster NGC 6366, using a wide field CCD camera at the prime focus of the Isaac Newton Telescope (INT 2.5m). The mean internal accuracy of the present V magnitudes and (B-V) colours ranges from 0.005mag for the stars at the top of the Red Giant Branch to 0.07mag for the
    Alonso, A. et al.

    Fecha de publicación:

    7
    1997
    Número de citas
    20
  • Brown dwarfs in the Pleiades cluster. II. J, H and K photometry.
    We have obtained near-infrared observations of some of the faintest objects so far known towards the Pleiades young stellar cluster, with the purpose of investigating the sequence that connects cluster very low-mass stars with substellar objects. We find that infrared data combined with optical magnitudes are a useful tool to discriminate cluster
    Zapatero Osorio, M. R. et al.

    Fecha de publicación:

    7
    1997
    Número de citas
    46
  • Atmospheric NLTE-models for the spectroscopic analysis of luminous blue stars with winds.
    We present a new, fast and easy to use NLTE line formation code for ``unified atmospheres'' with spherical extension and stellar winds, developed for the (routine) spectroscopic analysis of luminous blue stars, covering the spectral range from ``A'' to ``O'' and including central stars of planetary nebulae. The major features of our code are: Data
    Santolaya-Rey, A. E. et al.

    Fecha de publicación:

    7
    1997
    Número de citas
    288
  • A New Chemo-evolutionary Population Synthesis Model for Early-Type Galaxies. II. Observations and Results
    We present the results of applying a new chemo-evolutionary stellar population model, developed in a previous paper, to new high-quality observational data of the nuclear regions of two representative elliptical galaxies and the bulge of the Sombrero galaxy. Here we fit in detail ~20 absorption lines and six optical and near-infrared colors
    Vazdekis, A. et al.

    Fecha de publicación:

    7
    1997
    Número de citas
    190