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Past and Future Evolution of Sakurai's Object

Published online by Cambridge University Press:  26 May 2016

Falk Herwig
Falk Herwig*
Affiliation:
University of Victoria, Victoria, BC, Canada; fherwig@uvastro.phys.uvic.ca

Abstract

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We present a stellar evolution model sequence of the past and future evolution of the post-AGB born again star Sakurai's object (V 4334 Sgr). In order to match the short evolutionary time scale we have to assume that the convective ingestion of hydrogen-rich envelope material into the He-flash convection zone proceeds slower than predicted by the mixing length theory. For the future we predict a swift second evolution through the central star region before a second born-again evolution occurs.

Information

Type
Part III: Planetary Nebulae in the Scheme of Stellar Evolution
Information
Symposium - International Astronomical Union , Volume 209: Planetary Nebulae: Their Evolution and Role in the Universe , 2003, pp. 111 - 112
Copyright
Copyright © Astronomical Society of the Pacific 2003 

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