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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  • Two numerical processes for the calibration of photographic plates
    Not Available
    Collados, M. et al.

    Fecha de publicación:

    8
    1984
    Número de citas
    9
  • Nova Vulpeculae 1984
    IAUC 3977 available at Central Bureau for Astronomical Telegrams. IAUC 3977 available at Central Bureau for Astronomical Telegrams.
    Maley, P. et al.

    Fecha de publicación:

    8
    1984
    Número de citas
    0
  • Use of high resolution IUE spectra of MG 2 in cool stars to probe the local interstellar medium
    It is shown that, given suitable radial velocity values for the stars and the local interstellar medium (LISM) interstellar absorption can be distinguished from chromospheric self absorption within the MgII emissions from late type stars. Beta Hyi (G2IV) offers a clear example. Zeta Tuc (G2V) and delta Pav (G8V) which are very close to beta Hyi
    Molaro, P. et al.

    Fecha de publicación:

    7
    1984
    Número de citas
    3
  • An upper limit to the Beryllium abundance in the population 2 star HD 140283 from a high resoluion IUE spectrum
    An IUE archive spectrum of HD 140283 has been analyzed in the region of the 3131 Å 9Be II resonance doublet. Close comparison of the observed and synthetic spectra yields no measurable Be, and a conservative upper limit of 3×10-12 for 9Be, which is one fourth solar, can be set. With this star, and with a previous population II star HD 76932
    Molaro, P. et al.

    Fecha de publicación:

    7
    1984
    Número de citas
    8
  • Velocity signal produced by the passage of active regions compared with observations
    A calibrated numerical simulation of seasons for which there are observations of the passage of active regions across the visible disk of the sun, generating a velocity signal that can be compared with the Claverie et al. (1982) observations, has yielded values of this signal for a complete solar cycle. The results obtained indicate that the
    Herrero, A. et al.

    Fecha de publicación:

    6
    1984
    Número de citas
    7