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 language | English |
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Pages (from-to) | 396-399 |
Number of pages | 4 |
Journal | Astrophysics and Space Science |
Volume | 6 |
Issue number | 3 |
DOIs | |
State | Published - Mar 1970 |