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Winds in the atmospheres of central stars of Planetary Nebulae

Published online by Cambridge University Press:  25 May 2016

R. P. Kudritzki ,
R. H. Mendez ,
J. Puls  and
J. K. McCarthy
R. P. Kudritzki
Affiliation:
Munich University Observatory
R. H. Mendez
Affiliation:
Munich University Observatory
J. Puls
Affiliation:
Munich University Observatory
J. K. McCarthy
Affiliation:
Department of Astronomy, California Institute of Technology

Extract

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For this review we have chosen to concentrate on recent progress concerning the model atmosphere analysis of stellar winds in central stars of planetary nebulae (CSPNs). Since there is another review in these proceedings (by W.R. Hamann) devoted specifically to Wolf-Rayet type CSPNs, we will not consider them here. The reader interested in recent work on windless model atmospheres applied to CSPNs is referred to reviews by Napiwotzki (1995) and Werner et al. (1996). There is also an interesting paper by Werner (1996) on the Balmer line problem.

Type
III. Central Stars
Information
Symposium - International Astronomical Union , Volume 180: Planetary Nebulae , 1997 , pp. 64 - 73
Copyright
Copyright © Kluwer 1997 

References

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