A Little Monster Fed by Its Neighbor ✛

Original: "Feeding The Little Monster: An Accreting Intermediate-Mass Black Hole In A Minor Merger Secondary Galaxy"
· Marko Mićić, Julia St. Pierre
arXiv:2609.02667v1 · 2026-09-02 · CC0 1.0 · 1 min
In a small galaxy, astronomers found a black hole that feeds on gas flowing from a larger companion.

In a small galaxy, there's a black hole being fed by its neighbor. The satellite galaxy is slowly merging with a larger galaxy, and gas from the companion falls toward the center, where the black hole resides. It's not a giant, but it's not a lightweight either: its mass ranges from 800 to 5,000 solar masses. The Chandra telescope watched it for 16 years and caught just 31 photons, but these rare visitors revealed that the black hole is eating.

An intermediate-mass black hole is a bridge between the small black holes born from stars and the giants at the centers of galaxies. Very few of these mid-sized black holes are known, so every discovery matters.

The photons arrive only in soft X-rays, like the warm glow of a lamp. That's how gas shines when it swirls around a black hole in a flat disk, like water in a funnel. The closer to the black hole, the hotter the gas, and from its temperature astronomers weighed the black hole itself. It turns out the black hole is feeding quite eagerly, but not at full throttle.

This case shows how small black holes grow: they get their meals from larger neighbors during galaxy mergers. Previously, this had only been seen in computer simulations, but now we have a real example. The method used to extract information from 31 photons will help find more such black holes in future surveys.

Chandra's total exposure of 6.6 million seconds is equivalent to 76 days of continuous observation. Yet the source yielded only about 31 useful photons, roughly one photon every 2.5 days.

Intermediate-mass black holes are a popular subject in science fiction, for example in the series 'Stargate Universe', where the crew of the ship Destiny uses such a black hole for recharging. This paper describes a real candidate that may resemble those that inspire screenwriters.

kT_{in,rest} = 1.2 \times \left(\frac{M_{\bullet}}{10 M_{\odot}}\right)^{-1/4} \dot{m}^{1/4} \; \text{keV}
The accretion disk temperature increases with accretion rate and decreases with black hole mass
M_{\bullet} = 1.44 \, kT_{in,rest}^2 \sqrt{\frac{10 L_X}{1.26 \times 10^{38}}} \; M_{\odot}
Black hole mass is determined from disk temperature and X-ray luminosity
\dot{m} = \sqrt{\frac{kT_{in,rest}^4 L_X}{10 \times 2.0736 \times 1.26 \times 10^{38}}}
Dimensionless accretion rate is computed from temperature and luminosity
Scientists
Stephen HawkingJacob BekensteinFritz ZwickyBernhard RiemannJoseph WeberKarl Schwarzschild
Concepts
ultraluminous x ray source intermediate mass black hole stellar mass black hole soft x ray microquasar mercury ultralight dark matter galactic bulge accretion rate seyfert galaxy infrared excess Chandrasekhar limit obscured quasar active galaxy quasar feedback galactic center quasistar red giant merger rate intracluster medium