Physics
Scientist
München, Univ., Munich, Germany
Technische Univ., Munich, Germany
München, Universität, Munich, Germany
Formation of hydrogen lines in the atmospheres of type II supernovae.
Fundamental parameters of galactic luminous OB stars. II. A spectroscopic analysis of HDE 226868 and the mass of Cygnus X-1.
Unified NLTE model atmospheres including spherical extension and stellar winds - Method and first results
Unified NLTE Model Atmospheres Including Spherical Extension and Stellar Winds - Part Four - Improved Line Transfer and Wind Contamination of H he Profiles
Unified NLTE model atmospheres including spherical extension and stellar winds, 4: Improved line transfer and wind contamination of H, He profiles
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