Merging between a Central Massive Black Hole and a Compact Stellar System: A Clue to the Origin of M31’[CLC]s[/CLC] Nucleus
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Reference22 articles.
1. Competition of supermassive black holes and galactic spheroids in the destruction of globular clusters
2. Stellar dynamics in the nuclei of M31 and M32 - Evidence for massive black holes?
3. The Centers of Early-Type Galaxies with HST. IV. Central Parameter Relations.
Cited by 6 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. Lopsided spiral galaxies;Physics Reports;2009-02
2. Self‐Gravitating Eccentric Disk Models for the Double Nucleus of M31;The Astrophysical Journal;2004-08-10
3. On the Formation of an Eccentric Disk via Disruption of a Bulge Core near a Massive Black Hole;The Astronomical Journal;2003-06
4. Assessing Formation Scenarios for the Double Nucleus of M31 Using Two-Dimensional Image Decomposition;The Astronomical Journal;2002-07
5. Orbital decay of satellites crossing an accretion disc;Astronomy & Astrophysics;2001-09
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