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- W1645384420 abstract "It appears that the relative number of β –Cephei variables among the early B stars is comparable to the fraction of the evolutionary lifetime spent in the secondary contraction and early shell-burning phases (Lesh and Aizenman 1973a) and it may therefore be of some interest to investigate possible instability mechanisms associated with hydrogen shell-burning in stars within the mass range of 10 to 15 M ⊙ (Lesh and Aizenman 1973b)." @default.
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- W1645384420 date "1974-09-01" @default.
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- W1645384420 title "Convective Instability of Hydrogen-Burning Shells in β–Cephei Stars" @default.
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- W1645384420 doi "https://doi.org/10.1017/s1323358000013849" @default.
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