Statistics of planetary nebulae with [WR] central stars

Details Statistics of planetary nebulae with [WR] central stars Statistics of planetary nebulae with [WR] central stars

Jan 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001ap%26ss.275...67g&link_type=abstract

Astrophysics and Space Science, v. 275, Issue 1/2, p. 67-78 (2001).

Astronomy and Astrophysics

Astrophysics

18

Scientific paper

The status of planetary nebulae with Wolf-Rayet type central stars ([WR] PN) remains one of the most important problems in the investigation of planetary nebulae. We cannot claim to understand the evolution of low and intermediate-mass stars without answering the question how [WR] PN are created. Analyzing the statistical properties of the whole population of [WR] PN and comparing them to other planetary nebulae (non-[WR] PN) brings important information on their origin and evolutionary status. In this article I will summarize our results of this type of studies and show what limits they put on the possible evolutionary routes of [WR] PN creation.

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