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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| Main Authors: | , |
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| Format: | Article |
| Language: | English |
| Published: |
IOP Publishing
2025-01-01
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| Series: | The Astrophysical Journal |
| Subjects: | |
| Online Access: | https://doi.org/10.3847/1538-4357/adc99f |
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