Spectral analysis of early-type stars using a genetic algorithm based fitting method
We present the first automated fitting method for the quantitative spectroscopy of O- and early B-type stars with stellar winds. The method combines the non-LTE stellar atmosphere code fastwind from Puls et al. (2005, A&A, 435, 669) with the genetic algorithm based optimization routine pikaia from Charbonneau (1995, ApJS, 101, 309), allowing for a
Mokiem, M. R. et al.
Fecha de publicación:
10
2005