Maximal masses of Fe56 and Ni56 stars

A. Kovetz*, G. Shaviv

*Corresponding author for this work

Research output: Contribution to journalArticlepeer-review

Abstract

Upper bounds are derived for the masses of pure Ni56 and Fe56 stars, which are dynamically stable with respect to photodisintegration. Possible effects on stellar evolution are discussed.

Original languageEnglish
Pages (from-to)396-399
Number of pages4
JournalAstrophysics and Space Science
Volume6
Issue number3
DOIs
StatePublished - Mar 1970

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