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Upper Mass Limits for Hydrogen-Rich Planetary Nebula Nuclei

Published online by Cambridge University Press:  25 April 2016

D. J . Faulkner  and
P. R. Wood
D. J . Faulkner
Affiliation:
Mount Stromio and Siding Spring Observatories, Australian National University
P. R. Wood
Affiliation:
Mount Stromio and Siding Spring Observatories, Australian National University
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Abstract

We have discovered a radiation levitation mechanism which, under certain circumstances, can remove the last vestiges of hydrogen-rich material from an incipient planetary nebula nucleus if its mass exceeds a critical value of about 0.85M⊙. This process may be responsible for the production of helium-rich planetary nuclei, and their progeny the DB white dwarfs.

Type
Contributions
Information
Publications of the Astronomical Society of Australia , Volume 6 , Issue 1 , 1985 , pp. 62 - 65
Copyright
Copyright © Astronomical Society of Australia 1985

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