Note on the evolution of massive stars

Autor: Andriesse, C. D.
Zdroj: Astrophysics and Space Science; January 1983, Vol. 89 Issue: 2 p401-406, 6p
Abstrakt: By use of the fluctuation theory the mass of the massive stars can be calculated from the ‘observed’ luminosity, effective temperature and mass-loss rate. These masses differ from those obtained by fits to the ‘conventional’ evolution-tracks and they are used to construct alternative evolution-tracks.
Databáze: Supplemental Index