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

  • Unresolved Wind-driven Shells and the Supersonic Velocity Dispersion in Giant H II Regions
    The presence of giant shells or loops in giant H II regions is clear witness to the mechanical energy input from massive stars. Here we evaluate the impact that winds may have on the structure of giant nebulae and on their supersonic velocity dispersion. We follow the recent suggestion of Chu and Kennicutt to see whether a combination of a large
    Tenorio-Tagle, G. et al.

    Fecha de publicación:

    1
    1996
    Número de citas
    25
  • The Superluminal Source GRS 1915+105: A High Mass X-ray Binary?
    We obtained K-band (2.0-2.5 micron) infrared spectra of the visually obscured superluminal source GRS 1915+105 on three different epochs of the year 1995, at times when it was detected as a hard X-ray source. The three spectra exhibit HI Br(gamma) (2.167 micron) and HeI (2.058 micron) emission lines. The spectral morphology, absolute magnitude, and
    Mirabel, I. F. et al.

    Fecha de publicación:

    1
    1996
    Número de citas
    0
  • The Leonid Outburst of 1996
    There is strong anticipation that the Leonid meteor shower could produce storm-level activity in 1998 and/or 1999. The well-documented Leonid outburst in 1996 and the more poorly observed one in 1994 have been taken by many observers to imply that a storm is imminent, This article explores the possible relationship between the 1996 outburst in
    Kidger, Mark R.

    Fecha de publicación:

    1
    1996
    Número de citas
    0
  • Stars approaching the substellar limit in the α Persei open cluster.
    We present intermediate dispersion optical spectroscopy for seven very low-mass stars in the α Per open cluster with spectral types between M3 and M6, including the brown dwarf candidate of Rebolo et al. (1992). Our radial velocity measurements are found to be generally consistent with the mean cluster velocity to within the measurement errors. Hα
    Zapatero-Osorio, M. R. et al.

    Fecha de publicación:

    1
    1996
    Número de citas
    29
  • O-star mass-loss and wind momentum rates in the Galaxy and the Magellanic Clouds Observations and theoretical predictions.
    A new, very fast approximate method is presented to determine mass-loss rates of O-stars from Halpha_ line profiles. The method uses H and HeII departure coefficients from unified model atmospheres parametrized in a simple way as function of wind velocity together with photospheric NLTE line profiles as the inner boundary condition for a
    Puls, J. et al.

    Fecha de publicación:

    1
    1996
    Número de citas
    514