Further Evidence for a Direct-Collapse Origin of the Supermassive Black Hole at the Center of the Infinity Galaxy
Pieter van Dokkum, Gabriel Brammer, Connor Jennings, Imad Pasha, Josephine F. W. Baggen

TL;DR
This study provides evidence supporting the hypothesis that the supermassive black hole at the center of the Infinity Galaxy formed from gas collapse during a galaxy collision, based on JWST observations and velocity measurements.
Contribution
It offers new observational evidence confirming the formation of a SMBH from gas collapse in a galaxy collision, challenging recoil ejection scenarios.
Findings
SMBH's velocity matches surrounding gas, indicating in-situ formation.
Both nuclei host active SMBHs, ruling out ejection scenarios.
Gas cloud is photo-ionized by an AGN-like object, supporting recent SMBH formation.
Abstract
The z=1.14 galaxy consists of two ringed nuclei with an active supermassive black hole (SMBH) in between them. The system is likely the result of a nearly face-on collision between two disk galaxies with massive bulges. In van Dokkum et al. (2025) we suggested that the SMBH may have formed from shocked and compressed gas at the collision site, in a runaway gravitational collapse. Here we test this hypothesis using newly obtained JWST NIRSpec IFU observations. We first confirm that the system has a cloud of gas in between the nuclei that is photo-ionized by an AGN-like object near its center. Next, we constrain the origin of the SMBH from its radial velocity. If it formed in the cloud its velocity should be similar to the surrounding gas, whereas it would be offset if the SMBH had escaped from one of the nuclei or were associated with a faint galaxy. We find that the radial…
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Taxonomy
TopicsBlack Holes and Theoretical Physics · Relativity and Gravitational Theory · Cosmology and Gravitation Theories
