Feeding the Little Monster: An Accreting Intermediate-mass Black Hole in a Minor Merger Secondary Galaxy
- 1University of Oklahoma
- 2Central Connecticut State University
Abstract
We report the discovery of a luminous supersoft X-ray source associated with the secondary galaxy in a 10:1 minor merger at z = 0.216. We identified the system in the 3D-HST survey and observed it serendipitously in more than 100 Chandra observations, providing a combined exposure of 6.6 Ms. The secondary galaxy ( log ( M * / M ⊙ ) = 8.24) exhibits X-ray emission detected exclusively below 2.0 keV, with no significant hard-band photons. Because the source is low count, we characterize its spectrum using Bayesian hardness-ratio analysis combined with simulations of physically motivated spectral models folded through the Chandra response files. The observed count rates and hardness ratios are reproduced by a thermal accretion-disk spectrum with rest-frame inner-disk temperatures kT in = 0.18–0.30 keV and luminosities log( L X /erg s ⁻¹ ) = 40.5–41.2. Interpreted using a standard thin-disk framework, these properties imply a black hole mass of M • ≈ 8 × 10 ² –5 × 10 ³ M ⊙ accreting at ≈0.2–0.5 of the Eddington rate. Alternative interpretations involving ultraluminous X-ray supersoft sources are disfavored by the source’s luminosity, temperature, and lack of variability, and the host galaxy’s low star-formation rate. Numerical simulations predict that black holes in smaller, secondary galaxies could experience episodic rapid growth during minor mergers. This discovery provides observational support for this scenario and suggests that minor interactions may be an important channel for assembling supermassive black holes (SMBHs) in dwarf galaxies.
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BibTeX
@article{micic2026feeding,
title = {{Feeding the Little Monster: An Accreting Intermediate-mass Black Hole in a Minor Merger Secondary Galaxy}},
author = {Marko Mićić and Julia St. Pierre},
journal = {The Astrophysical Journal},
year = {2026},
month = oct,
doi = {10.3847/1538-4357/aea28c},
url = {https://iopscience.iop.org/article/10.3847/1538-4357/aea28c},
note = {CC BY 4.0},
}
RIS
TY - JOUR
TI - Feeding the Little Monster: An Accreting Intermediate-mass Black Hole in a Minor Merger Secondary Galaxy
AU - Marko Mićić
AU - Julia St. Pierre
PY - 2026
DA - 2026/10/14
JO - The Astrophysical Journal
DO - 10.3847/1538-4357/aea28c
UR - https://iopscience.iop.org/article/10.3847/1538-4357/aea28c
AB - We report the discovery of a luminous supersoft X-ray source associated with the secondary galaxy in a 10:1 minor merger at z = 0.216. We identified the system in the 3D-HST survey and observed it serendipitously in more than 100 Chandra observations, providing a combined exposure of 6.6 Ms. The secondary galaxy ( log ( M * / M ⊙ ) = 8.24) exhibits X-ray emission detected exclusively below 2.0 keV, with no significant hard-band photons. Because the source is low count, we characterize its spectrum using Bayesian hardness-ratio analysis combined with simulations of physically motivated spectral models folded through the Chandra response files. The observed count rates and hardness ratios are reproduced by a thermal accretion-disk spectrum with rest-frame inner-disk temperatures kT in = 0.18–0.30 keV and luminosities log( L X /erg s ⁻¹ ) = 40.5–41.2. Interpreted using a standard thin-disk framework, these properties imply a black hole mass of M • ≈ 8 × 10 ² –5 × 10 ³ M ⊙ accreting at ≈0.2–0.5 of the Eddington rate. Alternative interpretations involving ultraluminous X-ray supersoft sources are disfavored by the source’s luminosity, temperature, and lack of variability, and the host galaxy’s low star-formation rate. Numerical simulations predict that black holes in smaller, secondary galaxies could experience episodic rapid growth during minor mergers. This discovery provides observational support for this scenario and suggests that minor interactions may be an important channel for assembling supermassive black holes (SMBHs) in dwarf galaxies.
SN - 0004-637X
SN - 1538-4357
ER -