dorsal/arxiv
View SchemaOn the Physical Origins of the Millimeter Fundamental Plane in Active Galactic Nuclei
| Authors | Kratika Mazde, Angelo Ricarte, George N. Wong |
|---|---|
| Categories | |
| ArXiv ID | 2601.10612vv1 |
| URL | https://arxiv.org/abs/2601.10612 |
| License | http://creativecommons.org/licenses/by/4.0/ |
Abstract
Observations of active galactic nuclei have revealed a correlation between millimeter luminosity, X-ray luminosity, and mass, suggesting the emission in each of these bands is powered by a common source. Starting with a set of five general relativistic magnetohydrodynamic simulations with dynamically important magnetic fields, we perform ray-tracing calculations to produce spectra including synchrotron emission, bremsstrahlung emission, and Compton scattering. Our models with similar Eddington ratios to the objects for which the relationship was inferred naturally reproduce observations without tuning. Our lower Eddington ratio models depart from this relationship, likely attributable to an observational bias against extremely low accretion rates. We find that inverse Compton scattering dominates the production of X-rays over bremsstrahlung radiation in almost all models, and in all models consistent with the observed correlation. We find only a modest spin dependence in this relationship. This study demonstrates that a compact, hot accretion flow with dynamically important magnetic fields can naturally explain observed millimeter and X-ray properties in low-luminosity active galactic nuclei. Future work should explore the impacts of non-thermal electron populations, weaker magnetic fields, and radiative cooling.
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"abstract": "Observations of active galactic nuclei have revealed a correlation between millimeter luminosity, X-ray luminosity, and mass, suggesting the emission in each of these bands is powered by a common source. Starting with a set of five general relativistic magnetohydrodynamic simulations with dynamically important magnetic fields, we perform ray-tracing calculations to produce spectra including synchrotron emission, bremsstrahlung emission, and Compton scattering. Our models with similar Eddington ratios to the objects for which the relationship was inferred naturally reproduce observations without tuning. Our lower Eddington ratio models depart from this relationship, likely attributable to an observational bias against extremely low accretion rates. We find that inverse Compton scattering dominates the production of X-rays over bremsstrahlung radiation in almost all models, and in all models consistent with the observed correlation. We find only a modest spin dependence in this relationship. This study demonstrates that a compact, hot accretion flow with dynamically important magnetic fields can naturally explain observed millimeter and X-ray properties in low-luminosity active galactic nuclei. Future work should explore the impacts of non-thermal electron populations, weaker magnetic fields, and radiative cooling.",
"arxiv_id": "2601.10612",
"authors": [
"Kratika Mazde",
"Angelo Ricarte",
"George N. Wong"
],
"categories": [
"astro-ph.HE"
],
"license": "http://creativecommons.org/licenses/by/4.0/",
"title": "On the Physical Origins of the Millimeter Fundamental Plane in Active Galactic Nuclei",
"url": "https://arxiv.org/abs/2601.10612",
"version": "v1"
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