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

  • Stellar Kinematics and Chemical Abundances at the Thick-Disk/Halo Interface
    The old stellar populations of the Milky Way carry the signature of their formation environment and dynamical history in their kinematics and chemical abundances. In particular, the dynamically hot thick disk and halo contain the oldest stars in the Galaxy, and are remnants of its more chaotic past. We present a study of the high-latitude thick
    Rockosi, C. M. et al.

    Fecha de publicación:

    12
    2004
    Número de citas
    0
  • Stellar distribution in the Galactic disc from NIR color-magnitude diagrams
    We analyze the stellar distribution in the Galactic disc via NIR color-magnitude diagrams (CMDs). Extinction measurements in the K band are also extracted from the diagrams both for supporting stellar counts predictions of the Besançon and "SKY" models and for comparing with a three dimensional model of the Galactic extinction. The method is based
    Cabrera-Lavers, A. et al.

    Fecha de publicación:

    12
    2004
    Número de citas
    0
  • Star Formation in Satellite Galaxies
    The study of satellite galaxies can provide information on the merging and aggregation processes which, according to the hierarchical clustering models, form the larger spiral galaxies we observe. With the aim of testing hierarchical models of galaxy formation, we have conducted an observational program which comprises H$alpha$ imaging for both the
    Funes, José G. et al.

    Fecha de publicación:

    12
    2004
    Número de citas
    1
  • SSSPM J1444-2019: An extremely high proper motion, ultracool subdwarf
    We present the discovery of a new extreme high proper motion object (˜3.5 arcsec/year) which we classify as an ultracool subdwarf with [M/H] ˜ -0.5. It has a formal spectral type of sdM9 but also shows L-type features: while the VO bands are completely absent, it exhibits extremely strong TiO absorption in its optical spectrum. With a radial
    Scholz, R.-D. et al.

    Fecha de publicación:

    12
    2004
    Número de citas
    43
  • Some Spectroscopic Methods for Astrophysical Plasma Research
    Here we will present some spectroscopic methods for emission gas research in the emission line region of Active Galactic Nuclei (AGNs): (1) We will demonstrate the possibility to use the Boltzmann-plot method to estimate the physical conditions in the broad line regions (BLRs) (2) We will discuss the applicability of so called ``Gaussian method''
    Popović, L. Č. et al.

    Fecha de publicación:

    12
    2004
    Número de citas
    4
  • Simulations for the Permanent All Sky Survey (PASS) Experiment
    Simulations for PASS (Permanent All Sky Survey) are shown, which include the generation of artificial CCD images and photometric extraction of the stellar sources. First results indicate that PASS can obtain photometry with sufficient precision to pursue its principal goal, the detection of giant planet transits for all stars up to 11th mag.
    Deeg, H. et al.

    Fecha de publicación:

    12
    2004
    Número de citas
    0