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Paper: Properties of [WC] Planetary Nebulae
Volume: 391, Hydrogen-Deficient Stars
Page: 165
Authors: Górny, S.K.
Abstract: 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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