Astronomy and Astrophysics – Astronomy
Scientist
Astronomy and Astrophysics
Astronomy
Scientist
München, Universität, Munich, Germany
A non-LTE stellar atmosphere study of nitrogen-rich early-type stars
NLTE-Analysis of the Hot Helium-Rich Subdwarfs in the Palomar Green Survey
Non-LTE line formation in early B and late O stars. III - Singly ionized carbon
Quantitative spectroscopy of B supergiants in the Galaxy, the LMC and the SMC. I - The B0.5 IA supergiants Kappa Orionis, SK - 68 deg 41 and SK 159
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