Abstract
We self-consistently obtain shock locations in an accretion flow by using an analytical method. One can obtain the spectral properties, quasi-periodic oscillation frequencies and the outflow rates when the inflow parameters are known. Since temperature of the CENBOL decides the spectral states of the black hole, and also the outflow rate, the outflow rate is directly related to the spectral states.
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References
Chakrabarti, S. K. 1989,Ap. J.,347, 365.
Chakrabarti, S. K., Titarchuk, L. G. 1995,Ap. J. 455, 623.
Chakrabarti, S. K. 1996,Ap. J.,464, 664.
Chakrabarti, S. K. 1999,A&A,351, 185.
Corbelet al. 2001,Ap. J.,554, 43.
Das, S., Chattopadhayay, I., Chakrabarti, S. K. 2001a,Ap. J. 557, 983 (DCC01a)
Das, S, Nandi, A., Chattopadhayay, I, Chakrabarti, S. K. 2001b,A& A,379, 683 (DNCC01b)
Klein-Wolt, M.et al. 2001,ApSSS,276, 291.
Paczyński B., Wiita P. J., 1980,A&A,88, 23.
Smith, D. M., Heindl, W. A., Swank, J. H. 2002,Ap. J.,569, 362.
Smith, D. M., Heindl, W. A., Markwardt, W. A., Swank, J. H. 2001,Ap. J.,554L, 41.
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Das, S., Chakrabarti, S.K. Standing shocks around black holes and estimation of outflow rates. J Astrophys Astron 23, 143–147 (2002). https://doi.org/10.1007/BF02702479
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DOI: https://doi.org/10.1007/BF02702479