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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  • A Comparative Study of the Microvariability Properties in Radio-loud and Radio-quiet Quasars
    We have performed photometric optical observations of a sample of 17 core-dominated radio-loud quasars (CRLQs) and 17 radio-quiet quasars (RQQs). The aims were to confirm the existence of microvariations in strictly radio-quiet objects and to compare the properties of the variations in both types of quasars. Great care was taken to avoid selection
    de Diego, J. A. et al.

    Fecha de publicación:

    7
    1998
    Número de citas
    69
  • Three-dimensional P-wave velocity structure of Mt. Etna, Italy
    The three-dimensional P-wave velocity structure of Mt. Etna is determined to depths of 15 km by tomographic inversion of first arrival times from local earthquakes recorded by a network of 29 permanent and temporary seismographs. Results show a near-vertical low-velocity zone that extends from beneath the central craters to a depth of 10 km. This
    Villaseñor, A. et al.

    Fecha de publicación:

    6
    1998
    Número de citas
    52
  • The Solar Rotation Rate Ω(R, θ)
    In recent years, the capability to detect and analyse solar oscillation acoustic modes has greatly improved. The development of ground based networks like GONG or BiSON and the use of space platforms like SOHO has allowed us to study the structure and dynamics of the Sun with unprecedented precision.
    Eff-Darwich, A. et al.

    Fecha de publicación:

    6
    1998
    Número de citas
    0
  • The Most Luminous Stars in Our Galaxy
    We present quantitative analyses of 7 galactic O stars of spectral types from O3 to O6. By means of classical hydrostatic and planeparallel models we find the so-called He and Mass Discrepancies for a number of stars of our sample. We also prove the need of line-blocking for the correct reproduction of these spectra. For stars with effective
    Villamariz, M. R. et al.

    Fecha de publicación:

    6
    1998
    Número de citas
    0