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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  • The location of optically thin CO emission in M82
    Observations of a broad area at the core of M82, obtained with spatial resolution 30 arcsec and velocity resolution 15.6 km/sec in the J = 2-1 line of CO using the 12-m NRAO antenna at KPNO, are reported. The data are presented in graphs and contour maps and characterized in detail. It is found that the J = 2-1 map is similar to the J = 1-0 map of
    Phillips, J. P. et al.

    Fecha de publicación:

    6
    1989
    Número de citas
    0
  • The Local Interstellar Medium - A test-bed for the galactic ISM
    A method to explore the column density of the Local Interstellar Medium (LISM) using absorptions in the resonance H and K lines of Mg II. The intrinsic strengths of these lines in the temperature and density conditions prevailing in warm clouds in the LISM allows them to be used to explore many lines of sight where lines such a NaD and Ca II H and
    Genova, R. et al.

    Fecha de publicación:

    6
    1989
    Número de citas
    2
  • The G-dwarf problem - A tentative analytical approach, relaxing instantaneous recycling
    The general solution for the birth function B(m,t) of stars, derived by Casuso et al. (1989) was used to obtain a first-order analytical approximation to this function as a function of metallicity Z. This approximation was used to obtain a fit to the observational curve compiled by Tinsley (1980) for the cumulative function of stars with
    Casuso, E. et al.

    Fecha de publicación:

    6
    1989
    Número de citas
    3
  • The contribution to population in ellipticals of blue stragglers - A test of their origin
    An observational test of the binary hypothesis for the origin of the blue straggler (BS) stars has been performed searching for radial velocity variables among 27 BS in five galactic clusters. The significance of the BS phenomenon for the interpretation of evolutionary synthesis models and the spectra of elliptical galaxies is briefly discussed.
    Manteiga, Minia et al.

    Fecha de publicación:

    6
    1989
    Número de citas
    5
  • Physical parameters of reflection nebulae in the galaxy
    Given observed equivalent widths of Mg II and Mg I absorptions due to an interstellar cloud in which a late-B star is embedded, it is shown that the basic physical parameters (kinetic temperature, mean density, electron density, and radius) can be constrained. Hydrogen ionization by means of cosmic rays and the effect of the stellar radiation field
    Centurion, M. et al.

    Fecha de publicación:

    6
    1989
    Número de citas
    0
  • Observations of solar p-modes with L of not greater than 5
    Results are presented for the sun's radial velocity in integrated sunlight. A resonant scattering spectrometer has been used to determine the frequencies and amplitudes of p-modes with spherical harmonics of degree (l) of less than 3, and a second spectrophotometer, which observes part of the sun by means of a spatial filter, has been used to
    Palle, P. L. et al.

    Fecha de publicación:

    6
    1989
    Número de citas
    15