Photometry and Kinematics of Self-gravitating Eccentric Nuclear Disks

The Andromeda galaxy hosts an elongated nucleus with (at least) two distinct brightness peaks. The double nucleus can be explained by the projection of a thick, apsidally aligned eccentric nuclear disk of stars in orbit about the central black hole. Several nearby early-type galaxies have similar as...

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Bibliographic Details
Published in:The Astrophysical journal 2021-10, Vol.920 (2), p.149
Main Authors: Wernke, Heather N., Madigan, Ann-Marie
Format: Article
Language:English
Subjects:
Andromeda Galaxy
Astrophysics
Black holes
Disks
Galaxies
Galaxy nuclei
Gravitation
Image classification
Kinematics
Line of sight
Nuclei
Photometry
Simulation
Supermassive black holes
Velocity
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Summary:The Andromeda galaxy hosts an elongated nucleus with (at least) two distinct brightness peaks. The double nucleus can be explained by the projection of a thick, apsidally aligned eccentric nuclear disk of stars in orbit about the central black hole. Several nearby early-type galaxies have similar asymmetric nuclear features, indicating the possible presence of eccentric nuclear disks. We create simulated photometric (surface density) and kinematic (line-of-sight velocity) maps of eccentric nuclear disks using N -body simulations. We image our simulations from various lines of sight in order to classify them as double nuclei, offset nuclei, and centered nuclei. We explore the effects of mass segregation on the photometric maps, finding that heavier stars are concentrated in the brighter peak. The average line-of-sight velocity values are lower in an eccentric nuclear disk than for a circular ring about the supermassive black hole. The velocity dispersion values are higher and peak at the position of the supermassive black hole, which does not typically match the peak in photometry.
ISSN:0004-637X
1538-4357
DOI:10.3847/1538-4357/ac19ad