| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 1779128 | New Astronomy | 2013 | 13 Pages |
Abstract
⺠The accretion disk oscillations excites QPOs in the X-ray fluxes. ⺠The shocks may possibly be excite the oscillations in the accretion disk. ⺠We find the vertical to radial oscillation frequencies ratios are close to the 3:2. ⺠We determine the shock location in terms of flow parameters and black hole spin. ⺠We also estimate the possible spin of a few Galactic Micro-quasars from their QPOs.
Related Topics
Physical Sciences and Engineering
Physics and Astronomy
Astronomy and Astrophysics
Authors
Soumen Mondal, C.S. Choi,