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The critical mass for the overstability of massive zero-age main sequence stars
1988
Symposium - International astronomical union
Preserved Fulltext
The linear stability of massive extreme Pop I stars at the main sequence is investigated with a full nonadiabatic treatment. Contrary to earlier beliefs these stars become vibrationally unstable only beyond a critical mass as high as 440 M⊙ at the main sequence.
doi:10.1017/s0074180900158449
fatcat:2fhjdkfwvbharceifa6evo2tze