While there is strong evidence for clumping in the winds of massive hot stars, very little is known about clumping in the winds from Central Stars. We have checked [WC]-type CSPN winds for clumping by inspecting the electron-scattering line wings. At least for three stars we found indications for wind inhomogeneities.
| Identifer | oai:union.ndltd.org:Potsdam/oai:kobv.de-opus-ubp:1771 |
| Date | January 2007 |
| Creators | Todt, Helge, Hamann, Wolf-Rainer, Gräfener, G. |
| Publisher | Universität Potsdam, Mathematisch-Naturwissenschaftliche Fakultät. Institut für Physik und Astronomie |
| Source Sets | Potsdam University |
| Language | English |
| Detected Language | English |
| Type | InProceedings |
| Format | application/pdf |
| Rights | http://opus.kobv.de/ubp/doku/urheberrecht.php |
Page generated in 0.0019 seconds