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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  • The Kinematic Signature of the Sagittarius Dwarf Galaxy Tidal Debris from SDSS-DR1
    Recent results from the Sloan Digital Sky Survey (SDSS) and the 2MASS All-Sky Survey have clearly revealed the extent of the spatial distribution of stars affiliated with the tidal debris tail of the Sagittarius Dwarf Galaxy (Sgr). Although these surveys help to constrain the shape of the Sgr orbit, kinematics of the tidal tail stars are crucial in
    Wilhelm, R. et al.

    Fecha de publicación:

    12
    2003
    Número de citas
    0
  • The evolution of the Light Elements, Be and B (also Li), in the Galaxy
    We consider the evolution of the light elements, especially beryllium and boron but also lithium, in the Galaxy as derived from observations within 1 kpc of the Sun. The interest in Li has much to do with the evaluation of the universal baryon abundance via primordial nucleosynthesis, but the difficulties of interpretation have led to the need to
    Beckman, J. E. et al.

    Fecha de publicación:

    12
    2003
    Número de citas
    0
  • The Census of Planetary Nebulae in the Local Group
    We have been intensively searching for PNe in nearby galaxies as one of the main objectives of the Local Group Census (LGC). The LGC is a narrow-band survey of the galaxies of the Local Group observable from La Palma, that was awarded observing time during period two of the ING Wide Field Imaging Survey programme (http://www.ing.iac.es/WFS/)
    Corradi, R. L. M. et al.

    Fecha de publicación:

    12
    2003
    Número de citas
    0
  • Successful Measurement of the Full Magnetic Vector Near the Base of the Solar Corona
    The measurement of coronal fields has in the past generally been restricted to the field strength or to only some of the components of the magnetic vector. We present here a technique for measuring the full magnetic vector near the base of the solar corona. As an application we report on observations of a developing active region with ongoing
    Solanki, S. K. et al.

    Fecha de publicación:

    12
    2003
    Número de citas
    0
  • Starburst galaxy morphologies at z ˜ 0.04, z ˜ 0.5, and z ˜ 3
    One major difficulty in probing the nature of Lyman break galaxies (LBGs) at z ˜ 3 is the mismatch between our best images of LBGs, which are in the rest-UV, and the best images of local galaxies, which are in the rest-optical. To make direct comparisons between LBGs at z ˜ 3 and more local star-forming galaxies, we use HST/STIS to image a set of
    Durham, R. N. et al.

    Fecha de publicación:

    12
    2003
    Número de citas
    0
  • On the formation of massive stellar clusters
    Here we model a star forming factory in which the continuous creation of stars results in a highly concentrated, massive (globular cluster-like) stellar system. We show that under very general conditions a large-scale gravitational instability in the ISM, which triggers the collapse of a massive cloud, leads with the aid of a spontaneous first
    Tenorio-Tagle, G. et al.

    Fecha de publicación:

    12
    2003
    Número de citas
    19