An oscillating model suggestion for 63 Her | Zendy

Kiziloğlu N. | Zendy; Kirbiyik H. | Zendy; Civelek R. | Zendy

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An oscillating model suggestion for 63 Her

Author(s) -

Kiziloğlu N.,

Kirbiyik H.,

Civelek R.

Publication year - 2003

Publication title -

astronomische nachrichten

Language(s) - English

Resource type - Journals

SCImago Journal Rank - 0.394

H-Index - 63

eISSN - 1521-3994

pISSN - 0004-6337

DOI - 10.1002/asna.200310082

Subject(s) - physics , adiabatic process , astrophysics , stars , oscillation (cell signaling) , luminosity , asteroseismology , harmonic , thermodynamics , acoustics , galaxy , biology , genetics

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 ⊙ 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 ( l = 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 ⊙ .

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