TY  - JOUR
A1  - Reyes-Pérez, J.
A1  - Morisset, C.
A1  - Pena, M.
A1  - Mesa-Delgado, A.
T1  - A consistent spectral model of WR 136 and its associated bubble NGC 6888
T2  - Wolf-Rayet Stars : Proceedings of an International Workshop held in Potsdam, Germany, 1.–5. June 2015
N2  - We analyse whether a stellar atmosphere model computed with the code CMFGEN provides an optimal description of the stellar observations of WR 136 and simultaneously reproduces the nebular observations of NGC 6888, such as the ionization degree, which is modelled with the pyCloudy code. All the observational material available (far and near UV and optical spectra) were used to constrain such models. We found that the stellar temperature T∗, at τ = 20, can be in a range between 70 000 and 110 000 K, but when using the nebula as an additional restriction, we found that the stellar models with T∗ ∼ 70 000 K represent the best solution for both, the star and the nebula.
Y1  - 2015
UR  - https://publishup.uni-potsdam.de/frontdoor/index/index/docId/8827
UR  - https://nbn-resolving.org/urn:nbn:de:kobv:517-opus4-88274
SP  - 321
EP  - 324
ER  -