A Vertical Resonance of g-Mode Oscillations in Warped Disks and QPOs in Low-Mass X-Ray Binaries
Author(s) -
Shoji Kato
Publication year - 2005
Publication title -
publications of the astronomical society of japan
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 1.99
H-Index - 110
eISSN - 2053-051X
pISSN - 0004-6264
DOI - 10.1093/pasj/57.4.699
Subject(s) - polytropic process , physics , astrophysics , neutron star , resonance (particle physics) , polytrope , accretion (finance) , atomic physics
Resonant oscillations in warped disks are examined in order to explainhigh-frequency QPOs and horizontal-branch QPOs in low-mass X-ray binaries.Different from our previous work, addressed to the same subjects, we relax inthis paper the assumption that the disks are isothermal in the verticaldirection. That is, the pressure, density, and temperature are assumed to bedistributed in the vertical direction with a polytropic relation, and thepolytropic index changes as the disk state changes. By this generalization andby some subsidiaries we can qualitatively explain, within the framework of ourresonance model, observed large frequency variations in neutron-star QPOs andlittle variations in black-hole QPOs. We consider vertical resonances of g-modeoscillations, since they are most appropriate to explain observations.Comment: 11 pages, 3 figures, to be published in PASJ 57, Vol.
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