The 230 GHz Variability of Numerical Models of Sagittarius A*. II. The Physical Origins of the Variability

We continue our previous work, H.-S. Chan et al., to investigate how variations in the electron temperature prescription parameter, R _Low , influence the 3 hr variability at 230 GHz, M _Δ _T , in magnetically arrested disk (MAD) models of Sagittarius A* (Sgr A*), through analyzing a series of gener...

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Bibliographic Details
Main Authors: Ho-Sang Chan, Chi-kwan Chan
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astrophysical Journal
Subjects:
Online Access:https://doi.org/10.3847/1538-4357/adc99f
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