An oscillating model suggestion for 63 Her

Date

2003-01-01

Author

Kiziloglu, N
Kirbiyik, H
Civelek, R

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An attempt has been made towards explaining the observed frequencies in 63 Her. The evolution of rotating stars of 1.96, 1.98, 2.00, 2.05 and 2. 10 M-circle dot have been studied up to a point where stellar parameters match the observed luminosity and effective temperature of 63 Her. Radial and nonradial adiabatic oscillation frequencies were obtained in low harmonic degrees ( 1 = 0,1,2,3). One radial and three nonradial frequency values that match with the observed values were found for the model of mass 2.00 M-circle dot.

Subject Keywords

Space and Planetary Science, Astronomy and Astrophysics

URI

https://hdl.handle.net/11511/66857

Journal

ASTRONOMISCHE NACHRICHTEN

DOI

https://doi.org/10.1002/asna.200310082

Collections

Department of Physics, Article

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Citation Formats

N. Kiziloglu, H. Kirbiyik, and R. Civelek, “An oscillating model suggestion for 63 Her,” ASTRONOMISCHE NACHRICHTEN, pp. 215–218, 2003, Accessed: 00, 2020. [Online]. Available: https://hdl.handle.net/11511/66857.