Properties of [WC] Planetary Nebulae

Details Properties of [WC] Planetary Nebulae Properties of [WC] Planetary Nebulae

Jul 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aspc..391..165g&link_type=abstract

Hydrogen-Deficient Stars ASP Conference Series, Vol. 391, proceedings of the conference held 17-21 September, 2007, at Eberhard

Astronomy and Astrophysics

Astronomy

1

Scientific paper

The origin of the hydrogen deficient [WC] type central stars of planetary nebulae remains an open question in the theory of intermediate mass stars. In this review we present the results of the analysis concerning the nebulae surrounding these unusual nuclei. The properties of these nebulae bring important information on the evolutionary status of [WC] objects and constrain the possible theoretical scenarios.

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