Hostname: page-component-745bb68f8f-g4j75 Total loading time: 0 Render date: 2025-01-07T15:30:52.235Z Has data issue: false hasContentIssue false
  • English
  • Français

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; [email protected]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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.

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 

References

Asplund, M., Lambert, D. L., Kipper, T., Pollacco, D., & Shetrone, M. D. 1999, A&A, 343, 507 Google Scholar
Duerbeck, H. W., Liller, W., Sterken, C., et al. 2000, AJ, 119, 2360 CrossRefGoogle Scholar
Herwig, F. 2001, ApJ Lett., 554, L71 Google Scholar
Herwig, F., Blöcker, T., Langer, N., & Driebe, T. 1999, A&A, 349, L5 Google Scholar
Herwig, F. & Langer, N. 2001, Nucl. Phys. A, 688, 221, astro-ph/0010120 CrossRefGoogle Scholar
Iben, I. Jr. & MacDonald, J. 1995, in White Dwarfs, ed. Koester, D. & Werner, K., LNP No. 443 (Heidelberg: Springer), 48 Google Scholar