Proceedings of the 132nd Symposium of the International Astronomical Union, held in Paris, France, June 29-July 3, 1987This method is, however, restricted to a small region of the HR diagram containing suitable systems. ... and observed line profiles have been made only for the case of an Alfven wave driven wind model of or Ori (M2 lab) (Hartmann aamp;. Aa#39;:rettanbsp;...
|Title||:||The Impact of Very High S/N Spectroscopy on Stellar Physics|
|Author||:||International Astronomical Union. Symposium, G. Cayrel de Strobel, Monique Spite|
|Publisher||:||Springer Science & Business Media - 1988-04-30|