RADIAL PULSATIONS IN 63 HERCULIS

Date

1992-09-01

Author

UYANIKER, B

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Constructing a theoretical model of 1.88 M Q pulsation pro- perties of 63 Her have been analyzed. For the model, in question, pulsa- tion periods in the fundamental mode and first two overtones have been derived by solving the linearized pulsation equations. The model has been found to be vlbrationally stable

Subject Keywords

Astronomy and astrophysics

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https://hdl.handle.net/11511/64062

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Department of Physics, Conference / Seminar

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Citation Formats

B. UYANIKER, “RADIAL PULSATIONS IN 63 HERCULIS,” 1992, vol. 40, p. 736, Accessed: 00, 2020. [Online]. Available: https://hdl.handle.net/11511/64062.