Return to search

Tracking the Clumping in OB Stars from UV to radio

We review different line and continua diagnostics from the UV to radio, which can be utilized to simultaneously constrain the clumping structure throughout the stellar wind of massive OB stars.

Identiferoai:union.ndltd.org:Potsdam/oai:kobv.de-opus-ubp:1770
Date January 2007
CreatorsNajarro, F., Puls, Joachim, Herrero, A., Hanson, M. M., Martín-Pintado, J., Hillier, D. J.
PublisherUniversität Potsdam, Extern. Extern
Source SetsPotsdam University
LanguageEnglish
Detected LanguageEnglish
TypeInProceedings
Formatapplication/pdf
Rightshttp://opus.kobv.de/ubp/doku/urheberrecht.php

Page generated in 0.0021 seconds