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Gravity mode in gas-dust envelope of an oscillating star

Title
Gravity mode in gas-dust envelope of an oscillating star
Authors
Yang, JBastrukov, SMolodtsova, I
Ewha Authors
양종만
SCOPUS Author ID
양종만scopus
Issue Date
2005
Journal Title
NUOVO CIMENTO DELLA SOCIETA ITALIANA DI FISICA B-GENERAL PHYSICS RELATIVITY ASTRONOMY AND MATHEMATICAL PHYSICS AND METHODS
ISSN
1594-9982JCR Link
Citation
vol. 120, no. 10-11, pp. 1115 - 1122
Publisher
SOCIETA ITALIANA DI FISICA
Indexed
SCOPUS WOS scopus
Abstract
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.
DOI
10.1393/ncb/i2005-10143-y
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자연과학대학 > 물리학전공 > Journal papers
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