Sastri and Stothers 1974

Sastri, V.K., and R. Stothers, 1974: Influence of opacity on the pulsational stability of massive stars with uniform chemical composition. II. Modified Kramers opacity. Astrophys. J., 193, 677-678.

The pulsational stability of massive, chemically homogeneous stars of Population I has been investigated for a range of simple opacity representations consisting of a straight sum of electron-scattering and modified Kramers opacity. The critical mass for stability against nuclear-energized pulsations is found to be extraordinarily sensitive to small changes in the coefficient and/or temperature exponent of the absorption part of the opacity law. A gradual increase in the atomic absorption (dominant near the stellar surface) first raises the critical mass, then restricts the upper mass limit for instability, and finally eliminates pulsational instability at all masses.

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Sastri, V.K., and Stothers, R.: Influence of opacity on the pulsational stability of massive stars with uniform chemical composition. II. Modified Kramers opacity, Astrophys. J., 193, 677-678, 1974.

Sastri, V.K., and R. Stothers (1974), Influence of opacity on the pulsational stability of massive stars with uniform chemical composition. II. Modified Kramers opacity, Astrophys. J., 193, 677-678.

Sastri, V.K., and R. Stothers, 1974: Influence of opacity on the pulsational stability of massive stars with uniform chemical composition. II. Modified Kramers opacity. Astrophys. J., 193, 677-678.

Sastri, V.K., & Stothers, R. 1974, Astrophys. J., 193, 677.

Sastri VK, Stothers R. Influence of opacity on the pulsational stability of massive stars with uniform chemical composition. II. Modified Kramers opacity, Astrophys J 1974;193:677-678.

V.K. Sastri, R. Stothers, Astrophys. J. 193, 677-678 (1974).