Binary CSPN and PN Abundances

Details Binary CSPN and PN Abundances Binary CSPN and PN Abundances

Nov 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aipc..804..177f&link_type=abstract

PLANETARY NEBULAE AS ASTRONOMICAL TOOLS: International Conference on Planetary Nebulae as Astronomical Tools. AIP Conference Pr

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Planetary Nebulae, Binary Stars, Stellar Evolution, Planetary Nebulae, Binary And Multiple Stars, Stellar Structure, Interiors, Evolution, Nucleosynthesis, Ages

Scientific paper

Bipolar planetary nebulae (PNe) are often associated with high mass objects because of their metallicity, but there are numerous exceptions (including as many as 1/3 of all bipolars). On the other hand, it seems that the main requirement for this morphology is a binary companion. In this paper a possible connection of the exceptional cases to a specific binary evolution path is considered.

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