Stellar-mass black holes on the millimetre Fundamental Plane of black hole accretion

ABSTRACT Recent work revealed the existence of a galaxy ‘millimetre Fundamental Plane of black hole accretion’, a tight correlation between nuclear 1 mm luminosity, intrinsic 2–10 keV X-ray luminosity and supermassive black hole mass, originally discovered for nearby low- and high-luminosity active galactic nuclei. Here we use mm and X-ray data of five X-ray binaries (XRBs) to demonstrate that these stellar-mass black holes also lie on the mm Fundamental Plane, as they do at radio wavelengths. One source for which we have multi-epoch observations shows evidence of deviations from the plane after a state change, suggesting that the plane only applies to XRBs in the hard state, as is true again at radio wavelengths. We show that both advection-dominated accretion flows and compact jet models predict the existence of the plane across the entire range of black hole masses, although these models vary in their ability to accurately predict the XRB black hole masses.

Authors

Institutions

Publication Details

Journal
Monthly Notices of the Royal Astronomical Society
Published
2026-01-08
DOI
https://doi.org/10.1093/mnras/stag037
Primary Topic
Astrophysical Phenomena and Observations
Type
article
Field-Weighted Citation Impact
0.00

Funders

Controls
|||
ALL TIME
JAN
FEB
MAR
APR
MAY
JUN
JUL
AUG
SEP
OCT
article

Stellar-mass black holes on the millimetre Fundamental Plane of black hole accretion

Jindra Gensior, Martin Bureau, Ilaria Ruffa, Jacob S Elford et al.
Monthly Notices of the Royal Astronomical Society
Astrophysical Phenomena and Observations
article

Stellar-mass black holes on the millimetre Fundamental Plane of black hole accretion

Jindra Gensior, Martin Bureau, Ilaria Ruffa, Jacob S Elford, Hengyue Zhang, T. A. Davis, Thomas Williams, Rob Fender
article en

Abstract

ABSTRACT Recent work revealed the existence of a galaxy ‘millimetre Fundamental Plane of black hole accretion’, a tight correlation between nuclear 1 mm luminosity, intrinsic 2–10 keV X-ray luminosity and supermassive black hole mass, originally discovered for nearby low- and high-luminosity active galactic nuclei. Here we use mm and X-ray data of five X-ray binaries (XRBs) to demonstrate that these stellar-mass black holes also lie on the mm Fundamental Plane, as they do at radio wavelengths. One source for which we have multi-epoch observations shows evidence of deviations from the plane after a state change, suggesting that the plane only applies to XRBs in the hard state, as is true again at radio wavelengths. We show that both advection-dominated accretion flows and compact jet models predict the existence of the plane across the entire range of black hole masses, although these models vary in their ability to accurately predict the XRB black hole masses.

Monthly Notices of the Royal Astronomical SocietyVol. 546(2)
Arcetri Astrophysical Observatory (IT), University of Oxford (GB), Royal Observatory (GB), Cardiff University (GB), Universidad Diego Portales (CL), University of Edinburgh (GB)
National Science Foundation, National Aeronautics and Space Administration, California Institute of Technology, UK Research and Innovation, National Radio Astronomy Observatory, National Science Council, Korea Astronomy and Space Science Institute, National Astronomical Observatory of Japan, Jet Propulsion Laboratory, Science and Technology Facilities Council, National Institutes of Natural Sciences
Openalex Percentile: Top 91%
Astrophysical Phenomena and Observations
AI Navigator

Ask Laika to Summarize, Analyze, and Connect papers live on the map.

Summarize Papers & Methodologies

Extract key findings, datasets, and comparative methods across publications.

Benchmark Rankings & Visual Analytics

Rank top research institutions, authors, funders, topics, and journals by Field-Weighted Citation Impact (FWCI) and paper volume with instant charts.

Connect Distant Disciplines

Bridge topological clusters on the map to find hidden collaborative intersections.