TY  - JOUR
A1  - Kubátová, Brankica
A1  - Hamann, Wolf-Rainer
A1  - Todt, Helge Tobias
A1  - Sander, A.
A1  - Steinke, M.
A1  - Hainich, Rainer
A1  - Shenar, Tomer
T1  - Macroclumping in WR 136
T2  - Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.–5. June 2015
N2  - Macroclumping proved to resolve the discordance between different mass-loss rate diagnostics for O-type stars, in particular between Hα and the P v resonance lines. In this paper, we report first results from a corresponding investigation for WR stars. We apply our detailed 3-D Monte Carlo (MC) line formation code to the P v resonance doublet and show, for the Galactic WNL star WR136, that macroclumping is require to bring this line in accordance with the mass-loss rate derived from the emission-line spectrum.
Y1  - 2015
UR  - https://publishup.uni-potsdam.de/frontdoor/index/index/docId/8782
UR  - https://nbn-resolving.org/urn:nbn:de:kobv:517-opus4-87823
SP  - 125
EP  - 128
ER  -