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Ultramassive Black Holes in the Most Massive Galaxies: M-BH-sigma versus M-BH-R-b

Dullo, BT, Gil de Paz, A and Knapen, JH (2021) Ultramassive Black Holes in the Most Massive Galaxies: M-BH-sigma versus M-BH-R-b. Astrophysical Journal, 908 (2). ISSN 0004-637X

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We investigate the nature of the relations between black hole (BH) mass (MBH) and the central velocity dispersion (σ) and, for core-Sérsic galaxies, the size of the depleted core (Rb). Our sample of 144 galaxies with dynamically determined MBH encompasses 24 core-Sérsic galaxies, thought to be products of gas-poor mergers, and reliably identified based on high-resolution Hubble Space Telescope imaging. For core-Sérsic galaxies, i.e., combining normal-core (Rb < 0.5 kpc) and large-core galaxies (Rb ≳ 0.5 kpc), we find that MBH correlates remarkably well with Rb such that ${M}_{\mathrm{BH}}\propto {R}_{{\rm{b}}}^{1.20\pm 0.14}$ (rms scatter in log MBH of Δrms ∼ 0.29 dex), confirming previous works on the same galaxies apart from three new ones. Separating the sample into Sérsic, normal-core and large-core galaxies, we find that Sérsic and normal-core galaxies jointly define a single log-linear MBH–σ relation MBH ∝ σ4.88±0.29 with Δrms ∼ 0.47 dex; however, at the high-mass end, large-core galaxies (four with measured MBH) are offset upward from this relation by (2.5–4) × σs, explaining the previously reported steepening of the MBH–σ relation for massive galaxies. Large-core spheroids have magnitudes MV ≲ −23.50 mag, half-light radii Re ≳ 10 kpc, and are extremely massive, M* ≳ 1012 M☉. Furthermore, these spheroids tend to host ultramassive BHs (MBH ≳ 1010 M☉) tightly connected with their Rb rather than σ. The less popular MBH–Rb relation exhibits ∼62% less scatter in log MBH than the MBH–σ relations. Our findings suggest that large-core spheroids form via multiple major "dry" merger events involving super/ultramassive BHs, consistent with the flattening of the σ–LV relation observed at MV ≲ −23.5 mag.

Item Type: Article
Uncontrolled Keywords: Astronomy & Astrophysics; Physical Sciences; Science & Technology; Science & Technology; Physical Sciences; Astronomy & Astrophysics; astro-ph.GA; astro-ph.GA; astro-ph.CO; 0201 Astronomical and Space Sciences; 0202 Atomic, Molecular, Nuclear, Particle and Plasma Physics; 0306 Physical Chemistry (incl. Structural); Astronomy & Astrophysics
Subjects: Q Science > QB Astronomy
Divisions: Astrophysics Research Institute
Publisher: American Astronomical Society; IOP Publishing
SWORD Depositor: A Symplectic
Date Deposited: 21 Nov 2022 16:20
Last Modified: 21 Nov 2022 16:30
DOI or Identification number: 10.3847/1538-4357/abceae
URI: https://researchonline.ljmu.ac.uk/id/eprint/18174

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