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On the Relation of Core Mass by Chemical Composition in PN

Published online by Cambridge University Press:  07 August 2017

S.R. Pottasch*
Affiliation:
Kapteyn Laboratory P.O. Box 800 9700 AV Groningen The Netherlands

Abstract

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The attempts in the literature to find a relation between planetary nebula core mass and the nebular abundance ratios N/O and He/H are described. A critical discussion concludes that the evidence for such a relation is weak.

Type
V. Planetary Nebulae Connection: Evolution to White Dwarfs
Copyright
Copyright © Kluwer 1993 

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