The Physical Origin and Time Lag of Multifrequency Flares from Sgr A*

Sagittarius A*, the supermassive black hole at the center of our galaxy, exhibits flares across various wavelengths, yet its origin remains elusive. We performed 3D two-temperature general relativistic magnetohydrodynamic simulations of magnetized accretion flows initialized from multiloop magnetic...

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Bibliographic Details

Published in:	The Astrophysical Journal
Main Authors:	Hong-Xuan Jiang, Yosuke Mizuno, Indu K. Dihingia, Feng Yuan, Xi Lin, Christian M. Fromm, Antonios Nathanail, Ziri Younsi
Format:	Article
Language:	English
Published:	IOP Publishing 2025-01-01
Subjects:	Accretion Magnetohydrodynamics Magnetohydrodynamical simulations Low-luminosity active galactic nuclei Supermassive black holes Astrophysical black holes
Online Access:	https://doi.org/10.3847/1538-4357/adf1e5