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M = 1 instabilities in counter-rotating annuli in near Keplerian potentials - by Mher Vatche Kazandjian
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| dc.contributor.author | Kazandjian, Mher Vatche |
| dc.date.accessioned | 2012-06-13T07:14:01Z |
| dc.date.available | 2012-06-13T07:14:01Z |
| dc.date.issued | 2008 |
| dc.identifier.uri | http://hdl.handle.net/10938/7724 |
| dc.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 |
| dc.description | Bibliography : leaves 68-72. |
| dc.description.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 |
| dc.format.extent | x, 72 leaves : ill. 30 cm. |
| dc.language.iso | eng |
| dc.relation.ispartof | Theses, Dissertations, and Projects |
| dc.subject.classification | T:005166 AUBNO |
| dc.subject.lcsh | Astrophysics |
| dc.subject.lcsh | Galaxies |
| dc.subject.lcsh | Parallel processing (Electronic computers) |
| dc.title | M = 1 instabilities in counter-rotating annuli in near Keplerian potentials - by Mher Vatche Kazandjian |
| dc.type | Thesis |
| dc.contributor.department | American University of Beirut. Faculty of Arts and Sciences. Department of Physics |
