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S. Tsuruta, K. Fukumura (Montana State University)
Previous work on winds from the black hole magnetosphere in connection with rotation-powered AGN is extended to MHD accretion flows onto a supermassive black hole in the magnetosphere of an accretion-powered AGN. Fully general reltivistic treatment is applied. Shock formation in such accretion flows is investigated. The results will be reported. Possible observational implication will be discussed.
Previous | Session 118 | Next
Bulletin of the American Astronomical Society, 36 5
© 2004. The American Astronomical Society.