Clumping in the winds of O-type CSPNs
Recent studies of massive O-type stars present clear evidences of inhomogeneous and clumped winds. O-type (H-rich) central stars of planetary nebulae (CSPNs) are in some ways the low mass–low luminosity analogous of those massive stars. In this contribution, we present preliminary results of our on-...
| Main Authors: | , , |
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| Format: | Others |
| Language: | English |
| Published: |
Universität Potsdam
2007
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| Subjects: | |
| Online Access: | http://nbn-resolving.de/urn:nbn:de:kobv:517-opus-17801 http://opus.kobv.de/ubp/volltexte/2008/1780/ |