Past and future evolution of Sakurai's object

Falk Herwig

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arXiv · astro-ph/0202142

Past and future evolution of Sakurai's object

Falk Herwig

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Abstract

We present a stellar evolution model sequence of the past and future evolution of the post-AGB born again star Sakurai's object (V4334 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.

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Falk Herwig. 2002-02-06. Past and future evolution of Sakurai's object. https://arxiv.org/abs/astro-ph/0202142

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