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

  • WeCAPP - The Wendelstein Calar Alto Pixellensing Project Tracing Dark and Bright Matter in M31
    We present WeCAPP, a long term monitoring project searching for microlensing events towards M31. Since 1997 the bulge of M31 was monitored in two different wavebands with the Wendelstein 0.8 m telescope. In 1999 we extended our observations to the Calar Alto 1.23 m telescope. Observing simultaneously at these two sites we obtained a time coverage
    Riffeser, A. et al.

    Fecha de publicación:

    0
    2001
    Número de citas
    0
  • Water vapour measurements at the Observatorio del Roque de los Muchachos
    Not Available
    Kidger, M. R. et al.

    Fecha de publicación:

    0
    2001
    Número de citas
    0
  • Understanding Circumnuclear Star Formation in Spiral Galaxies
    We are attempting to learn the circumstances under which bursts of star formation may be triggered around the nuclei of many nearby spiral galaxies. By comparing the observed equivalent widths of the Brγ emission line and the CO(2-0) absorption band in each of the circumnuclear hotspots, with starburst models from the literature, we can place
    Ryder, S. D. et al.

    Fecha de publicación:

    0
    2001
    Número de citas
    0
  • Tidal Streams in the Galactic Halo: Evidence for the Sagittarius Northern Stream or Traces of a New Nearby Dwarf Galaxy
    Not Available
    Martínez-Delgado, D. et al.

    Fecha de publicación:

    0
    2001
    Número de citas
    1
  • The stellar populations of the Milky Way satellites: the early Universe through the color-magnitude diagram
    The Milky Way satellites offer the possibility of studying their star formation histories in great detail. Color-magnitude diagrams (CMDs) reaching the old main-sequence turnoffs, allow a careful modelling of their stellar populations using synthetic CMDs, and spectroscopy of the brightest stars, provides a direct measurement of their metallicity
    Gallart, Carme

    Fecha de publicación:

    0
    2001
    Número de citas
    0