Standing Shocks around Black Holes and Estimation of Outflow Rates

Details Standing Shocks around Black Holes and Estimation of Outflow Rates Standing Shocks around Black Holes and Estimation of Outflow Rates

Jun 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002japa...23..143d&link_type=abstract

Journal of Astrophysics and Astronomy, Vol. 23, p.143

Astronomy and Astrophysics

Astrophysics

1

Scientific paper

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 outflowrates 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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