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

A. Kovetz; D. Prialnik; G. Shaviv

doi:10.1007/BF00640366

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

A. Kovetz^*, D. Prialnik, G. Shaviv

^*Corresponding author for this work

Tel Aviv University

Research output: Contribution to journal › Article › peer-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 language	English
Pages (from-to)	463-476
Number of pages	14
Journal	Astrophysics and Space Science
Volume	37
Issue number	2
DOIs	https://doi.org/10.1007/BF00640366
State	Published - Oct 1975

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title = "Dynamic phases in the evolution of a 1.25 M⊙ C-O star",

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.",

author = "A. Kovetz and D. Prialnik and G. Shaviv",

year = "1975",

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

Abstract

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