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

  • Con árbitro
    The optical variability of 3C 345
    The behavior of the light curve of 3C 345 is analyzed using all B magnitudes available in the literature, thus extending the number of points in the compiled light curve of this object by a factor of more than 50 percent and the coverage by about 7 yrs, in comparison with the light curve compiled by Kidger and Beckman (1986). In addition, a new and
    Kidger, M. R.

    Fecha de publicación:

    12
    1989
    Bibcode
    1989A&A...226....9K
    Número de citas
    29
  • Sin árbitro
    Supernova 1989U in UGC 5295
    IAUC 4930 available at Central Bureau for Astronomical Telegrams. IAUC 4930 available at Central Bureau for Astronomical Telegrams.
    Lopez, R. et al.

    Fecha de publicación:

    12
    1989
    Bibcode
    1989IAUC.4930....2L
    Número de citas
    0
  • Sin árbitro
    Supernova 1989N in NGC 3646
    IAUC 4932 available at Central Bureau for Astronomical Telegrams. IAUC 4932 available at Central Bureau for Astronomical Telegrams.
    Lopez, R. et al.

    Fecha de publicación:

    12
    1989
    Bibcode
    1989IAUC.4932....2L
    Número de citas
    0
  • Con árbitro
    Quantitative spectroscopy of O-stars in the Magellanic Clouds. I - The young open cluster NGC 346 in the SMC
    Results are presented on a non-LTE analysis of high-resolution Cassegrain echelle CCD spectra of the four most luminous stars in the NGC 346 cluster in the SMC, obtained with the ESO 3.6-m telescope, making it possible to estimate the age of the NGC 346 cluster and to trace its evolution. The results yield the effective temperatures, gravities
    Kudritzki, R. P. et al.

    Fecha de publicación:

    12
    1989
    Bibcode
    1989A&A...226..235K
    Número de citas
    35
  • Con árbitro
    Oxygen abundances in unevolved metal-poor stars - Interpretation and consequences
    The oxygen abundance has been determined by analysis of the O I infrared triplet in 30 unevolved field stars of metallicities in the range Fe/H abundance ratio between -0.2 and -3.5. The data show that the O/Fe abundance ratio increases monotonically as metallicity decreases from solar, reaching values in the range 1.0-1.2 at an Fe/H abundance
    Abia, C. et al.

    Fecha de publicación:

    12
    1989
    Bibcode
    1989ApJ...347..186A
    Número de citas
    174