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Lense-Thirring QPO model testing by QPO phenomena in GX339-4 2010 outburst

Published online by Cambridge University Press:  21 February 2013

H. Q. Gao ,
J. L. Qu ,
Z. Zhang  and
J. N. Zhou
H. Q. Gao
Affiliation:
Institute of High Energy Physics, CAS, Beijing 100049, P.R. China email: [email protected]
J. L. Qu
Affiliation:
Institute of High Energy Physics, CAS, Beijing 100049, P.R. China email: [email protected]
Z. Zhang
Affiliation:
Institute of High Energy Physics, CAS, Beijing 100049, P.R. China email: [email protected]
J. N. Zhou
Affiliation:
Institute of High Energy Physics, CAS, Beijing 100049, P.R. China email: [email protected]
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Abstract

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Lense-Thirring QPO model is a promising model to explain QPO phenomena (Ingram et al. (2009)). In this model the QPO results from Lense-Thirring precession of a optical translucent inner hot flow in a truncated disc geometry. Now we check this model with different types QPO (see (Belloni et al. (2011)) for a recent review) of black hole transient (BHT) GX 339-4 2010 outburst and suggest type C QPOs are mainly coincident with this model prediction while type B QPOs are not.

Keywords

Black hole transientLense-Thirring precessionQuasi-periodic oscillations (QPO)
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 8 , Symposium S290: Feeding Compact Objects: Accretion on All Scales , August 2012 , pp. 211 - 212
Copyright
Copyright © International Astronomical Union 2013

References

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Motta, S., Munoz-Darias, T., Casella, P., Belloni, T., & Homan, J. 2011, MNRAS, 418, 2292Google Scholar