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Wind inhomogeneities in [Wc] central stars of planetary nebulae
Published online by Cambridge University Press: 26 May 2016
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In the present poster paper, we summarize the observational spectroscopic evidence for wind clumping originating in some [WC8-10] and [WO4] central stars of planetary nebulae. Specifically, we concentrate on the C iii λ5696 and C iv λλ5801/12 emission-line variability observed for well-known planetary nebula nuclei.
- Type
- Part 1. Atmospheres of Massive Stars
- Information
- Copyright
- Copyright © Astronomical Society of the Pacific 2003
References
Acker, A., Grosdidier, Y.
2002, in: Dopita, M.A., Kwok, S. & Sutherland, R.S. (eds.)
Planetary nebulae: their Evolution and Role in the Universe,
Proc. IAU Symp. No. 209, in press.CrossRefGoogle Scholar
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