Publications

This section contains the publications database that collects IAC articles published in scientific journals. Please, click on the arrow to see full search filter and sort options: author, journal, year, etc..

It also provides access to IAC Preprints Repository here: https://research.iac.es/preprints/

  • P Cygni: An Extraordinary Luminous Blue Variable
    P Cygni is a prototype for understanding mass loss from massive stars. This textbook star is known first of all because of two great eruptions in the 17th century. In the first half of this century it has given its name to a class of stars which are characterized by spectral lines consisting of nearly undisplaced emissions accompanied by a blue
    Israelian, G. et al.

    Advertised on:

    10
    1999
    Citations
    34
  • Jets, Knots, and Tails in Planetary Nebulae: NGC 3918, K1-2, and Wray 17-1
    We analyze optical images and high-resolution, long-slit spectra of three planetary nebulae that possess collimated, low-ionization features. NGC 3918 is composed of an inner, spindle-shaped shell mildly inclined with respect to the plane of the sky. Departing from the polar regions of this shell, we find a two-sided jet expanding with velocities
    Corradi, Romano L. M. et al.

    Advertised on:

    10
    1999
    Citations
    49
  • GALACTIC GLOBULAR CLUSTERS RELATIVE AGES: CLUES ON THE MILKY WAY FORMATION AND EVOLUTION
    El objetivo de esta tesis es el estudio de la historia de formación de nuestra Galaxia. Para ello, hemos analizado los sistemas estelares más viejos, los cúmulos globulares, obteniendo como resultado principal el que esa formación e produjo mediante un colapso rápido del halo. La tesis se presenta en tres bloques principales. -En el primero se
    ALFREDO RAFAEL ROSENBERG GONZALEZ

    Advertised on:

    10
    1999
  • Fundamental parameters of stars (Allende Prieto+, 1999)
    The Hipparcos mission has made it possible to constrain the positions of nearby field stars in the colour-magnitude diagram with very high accuracy. These positions can be compared with the predictions of stellar evolutionary calculations to provide information on the basic parameters of the stars: masses, radii, effective temperatures, ages, and
    Allende Prieto, C. et al.

    Advertised on:

    10
    1999
    Citations
    3