Dynamic phases in the evolution of a 1.25 M C-O star

Research output: Contribution to journalArticlepeer-review

Abstract

The evolution of a 1.25 M carbon and oxygen (equal fractions by mass) homogeneous star is followed by means of a computer code capable of dealing with dynamic evolutionary phases. After carbon ignition at the center, followed by successive shell flashes and the formation of a T-inversion, convection begins at the surface and the model evolves through a very short but strong dynamic phase (viz. a pulsation) after which it settles down to a white dwarf configuration.

Original languageEnglish
Pages (from-to)463-476
Number of pages14
JournalAstrophysics and Space Science
Volume37
Issue number2
DOIs
StatePublished - Oct 1975

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