Query : 2021MNRAS.502.4794N

2021MNRAS.502.4794N - Mon. Not. R. Astron. Soc., 502, 4794-4814 (2021/April-3)

Formation of the largest galactic cores through binary scouring and gravitational wave recoil.


Abstract (from CDS):

Massive elliptical galaxies are typically observed to have central cores in their projected radial light profiles. Such cores have long been thought to form through 'binary scouring' as supermassive black holes (SMBHs), brought in through mergers, form a hard binary and eject stars from the galactic centre. However, the most massive cores, like the ∼3 kpc core in A2261-BCG, remain challenging to explain in this way. In this paper, we run a suite of dry galaxy merger simulations to explore three different scenarios for central core formation in massive elliptical galaxies: 'binary scouring', 'tidal deposition', and 'gravitational wave (GW) induced recoil'. Using the GRIFFIN code, we self-consistently model the stars, dark matter, and SMBHs in our merging galaxies, following the SMBH dynamics through to the formation of a hard binary. We find that we can only explain the large surface brightness core of A2261-BCG with a combination of a major merger that produces a small ∼1 kpc core through binary scouring, followed by the subsequent GW recoil of its SMBH that acts to grow the core size. Key predictions of this scenario are an offset SMBH surrounded by a compact cluster of bound stars and a non-divergent central density profile. We show that the bright 'knots' observed in the core region of A2261-BCG are best explained as stalled perturbers resulting from minor mergers, though the brightest may also represent ejected SMBHs surrounded by a stellar cloak of bound stars.

Abstract Copyright: © 2021 The Author(s) Published by Oxford University Press on behalf of Royal Astronomical Society

Journal keyword(s): black hole physics - gravitational waves - methods: numerical - galaxies: interactions - galaxies: kinematics and dynamics - galaxies: nuclei

Simbad objects: 5

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Number of rows : 5
N Identifier Otype ICRS (J2000)
ICRS (J2000)
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2021
1 4C 74.13 BiC 07 41 44.449 +74 14 39.59   20.15 18.53     ~ 22 2
2 IC 1101 rG 15 10 56.100 +05 44 41.19   15.10       ~ 150 2
3 3C 338.0 QSO 16 28 38.2447110 +39 33 04.233634   12.78 11.78     ~ 719 5
4 2MASX J17222717+3207571 BiC 17 22 27.185 +32 07 57.25           ~ 39 1
5 ACO 2261 ClG 17 22 28.3 +32 09 13           ~ 305 0

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