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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  • Calibration and analysis of the GOLF experiment
    The solar core is the region where all the nuclear reactions take place and, therefore, where the energy is generated. Understanding the physics of these internal layers, the theory of solar and stellar structure can be settled into form grounds. However this is the most unknown region of the Sun. Helioseismology, mainly through the gravity modes
    García, R. A.

    Fecha de publicación:

    8
    1996
    Número de citas
    7
  • An ellipsoidal modulation in X-ray Nova VELA 1993
    Observations of the soft X-ray transient Nova Vela 1993 are presented. These are the first observations, taken during quiescence in 1995 and 1996. An orbital, ellipsoidal modulation is found in the R-band photometry (mean magnitude of 20.6), with an amplitude of 0.23 mags at 6.86 +/- 0.12 h. The H-alpha emission spectra is presumed to arise from
    Shabbaz, T.. et al.

    Fecha de publicación:

    8
    1996
    Número de citas
    0
  • TOWARDS THE UNDERSTANDING OF THE STELLAR POPULATIONS OF THE EARLY-TYPE GALAXIES
    EL OBJETIVO DE ESTA TESIS ES EL ESTUDIO DE LOS DIFERENTES PARAMETROS QUE DEFINEN LAS POBLACIONES ESTELARES DE LAS GALAXIAS. PARA ELLO SE DESARROLLA UN INNOVADOR MODELO DE SINTESIS DE POBLACIONES ACTUALIZADO CON LOS ULTIMOS AVANCES EN LA MATERIA. CON ESTE MODELO SE PREDICEN UN GRAN NUMERO DE OBSERVABLES (COLORES E INDICES) QUE SE COMPARAN CON DATOS
    ALEXANDRE VAZDEKIS VAZDEKIS

    Fecha de publicación:

    7
    1996
  • The microvariability characteristics of OJ 287.
    We present the results of the study of visible (UBVRIZ) intra-night microvariability in the blazar OJ 287. Useful observations (at least four integrations in a single band in a single night with a single telescope) were carried out on a total of 26 nights from November 1993 to November 1994. Relative photometry was taken against star 4, 10 and 11
    Gonzalez-Perez, J. N. et al.

    Fecha de publicación:

    7
    1996
    Número de citas
    13
  • The mass of the black hole in GS 2000+25 (=QZ Vul).
    The authors report the first infrared light curve of GS 2000+25. By modelling the brightness variations as ellipsoidal modulations of the secondary star, the authors find the mass of the compact object to lie between 4.8 and 14.4 Msun (90 per cent confidence) for secondary masses ≤0.7 Msun; this result is independent of the mass ratio, q. The upper
    Beekman, G. et al.

    Fecha de publicación:

    7
    1996
    Número de citas
    26
  • The luminosity function evolution of soft X-ray-selected active galactic nuclei in the RIXOS survey
    A sample of 198 soft X-ray-selected active galactic nuclei (AGN) from the ROSAT International X-ray Optical Survey (RIXOS) is used to investigate the X-ray luminosity function and its evolution. RIXOS, with a flux limit of 3x10^-14 erg s^-1 cm^-2 (0.5 to 2.0 keV), samples a broad range in redshift over 20 deg^2 of sky, and is almost completely
    Page, M. J. et al.

    Fecha de publicación:

    7
    1996
    Número de citas
    50