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
    Do all bright elliptical galaxies have active nuclei?
    The evidence is noted that (1) a flux density limited complete sample of X-ray emitting BL Lac type sources is now available from Schwartz and Ku (1983), that (2) the radio through X-ray emission of BL Lac type sources is most easily interpreted as nonthermal emission from a relativistically boosted jet pointed close to the line of sight and that
    Perez-Fournon, I. et al.

    Fecha de publicación:

    1
    1984
    Bibcode
    1984A&A...130L..13P
    Número de citas
    22
  • Sin árbitro
    El origen del sistema de cúmulos globulares de la galaxia Messier 87.
    Not Available
    Forte, J. C. et al.

    Fecha de publicación:

    0
    1984
    Bibcode
    1984BAAA...28...75F
    Número de citas
    0
  • Sin árbitro
    Book-Review - Infrared Astronomy - I.A.U. Symposium NO.96
    Not Available
    Wynn-Williams, C. G. et al.

    Fecha de publicación:

    12
    1983
    Bibcode
    1983Obs...103..296W
    Número de citas
    0
  • Con árbitro
    The age decay of stellar magnetic activity in MS field solar-type stars
    The age decay of two indicators of the stellar magnetic activity (λ2800 Mg II emission flux and λ10830 He I equivalent width) have been studied for field solar-type stars. The Li abundance has been used, in most of the cases, as a stellar age indicator. A calibrated decay law for Mg II has been determined and compared with a similar one, recently
    Cabestany, J. et al.

    Fecha de publicación:

    11
    1983
    Bibcode
    1983Ap&SS..97..151C
    Número de citas
    2
  • Con árbitro
    Are the small active regions related to the decay of the larger ones?
    According to several properties, the active regions are divided in two groups whose limit is roughly set at 1021 Mx. A statistical analysis indicates that the small regions emerge almost exclusively in the remnant magnetic regions, resulting from the decay of previous active centers. According to these facts, a tentative picture is proposed, where
    de la Rosa, I. G.

    Fecha de publicación:

    11
    1983
    Bibcode
    1983SoPh...89...51D
    Número de citas
    8