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Wind inhomogeneities in [Wc] central stars of planetary nebulae
Published online by Cambridge University Press: 26 May 2016
Extract
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
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- Copyright © Astronomical Society of the Pacific 2003