On the Formation of an Eccentric Disk via Disruption of a Bulge Core near a Massive Black Hole-Reference-Cited by-同舟云学术

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On the Formation of an Eccentric Disk via Disruption of a Bulge Core near a Massive Black Hole

Published:2003-06 Issue:6 Volume:125 Page:2998-3004
ISSN:0004-6256
Container-title:The Astronomical Journal
language:en
Short-container-title:Astron J

Author:

Quillen A. C.,Hubbard Alex

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference32 articles.

1. The Distribution of Stars near the Supermassive Black Hole in the Galactic Center

2. The M 31 double nucleus probed with OASIS and HST

3. Merging between a Central Massive Black Hole and a Compact Stellar System: A Clue to the Origin of M31’[CLC]s[/CLC] Nucleus

4. Gas Fueling and Nuclear Gaseous Disk Formation in Merging between a Central Massive Black Hole and a Gas Clump

5. Binney, J. & Tremaine, S. 1987, Galactic Dynamics (Princeton: Princeton Univ. Press)

Cited by 4 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. The doubling of stellar black hole nuclei;Monthly Notices of the Royal Astronomical Society;2013-02-18

2. Lopsided spiral galaxies;Physics Reports;2009-02

3. Accretion and Nuclear Activity of Quiescent Supermassive Black Holes. II. Optical Study and Interpretation;The Astrophysical Journal;2006-03-20

4. Self‐Gravitating Eccentric Disk Models for the Double Nucleus of M31;The Astrophysical Journal;2004-08-10

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