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Gravity mode in gas-dust envelope of an oscillating star
- Gravity mode in gas-dust envelope of an oscillating star
- Yang, J; Bastrukov, S; Molodtsova, I
- Ewha Authors
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- NUOVO CIMENTO DELLA SOCIETA ITALIANA DI FISICA B-GENERAL PHYSICS RELATIVITY ASTRONOMY AND MATHEMATICAL PHYSICS AND METHODS
- NUOVO CIMENTO DELLA SOCIETA ITALIANA DI FISICA B-GENERAL PHYSICS RELATIVITY ASTRONOMY AND MATHEMATICAL PHYSICS AND METHODS vol. 120, no. 10-11, pp. 1115 - 1122
- SOCIETA ITALIANA DI FISICA
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- The hydrodynamic mechanism of gravitational coupling between seismic vibrations of a star and fluctuations of gas-dust flows in stellar envelope is discussed. Working from a homogeneous model of a spherical stellar cocoon-a star embedded in a thick dusty shell, the self-consistent equations of hydro-gravity, formulated as a counterpart of equations of hydro-magnetic model of interstellar,gas-dynamics, are introduced. Particular attention is given to shear oscillations of ambient gas-dust matter triggered by seismic pulsations of a star owing its existence to circumstellar gravitational stresses. It is shown that, in the absence of accretion. the frequency of this gravity-driven mode in circumstellar envelope is proportional to the frequency of the g-mode in the star bulk. The implication of the model to a number of current astrophysical problems is briefly discussed.
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