Multi-level non-LTE calculations for very optically thick winds and photospheres under extreme NLTE conditions
A new technique to calculate multilevel non-LTE continuum formation in the UV of stellar winds and plane-parallel, static stellar atmospheres is developed using a local approximate lambda operator similar to those presented by Werner and Husfeld (1985) and Hamann (1986). In the present formulation, the iteration of the transfer equation solution is
Pauldrach, A. et al.
Fecha de publicación:
6
1988