M = 1 instabilities in counter-rotating annuli in near Keplerian potentials - by Mher Vatche Kazandjian
Abstract
Counter-rotating annuli around a super massive black hole were evolved using a f ully self-consistent N-body code, Gadget 2.0 . A small fraction of counter-rotat ing mass is required to drive the annuli unstable. These annuli develop into glo bal m = 1 pr
Description
Thesis (M.S.)--American University of Beirut, Dept. of Physics, 2008.;"Advisor : Dr. Jihad Touma, Associate Professor ,Physics--Member of Committee : Dr. Ghassan Antar, Assistant Professor, Physics--Member of Committee : Dr. Eid Mounib, Professor, Physics
Bibliography : leaves 68-72.
Bibliography : leaves 68-72.