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Global Structure of Accretion Flows in Sgr A*

Sagittarius A* (Sgr A*) is a compact radio source at the Galactic center. Observations have confirmed that its mass is approximately (4.1 ± 0.4) × 10 ^6 M _⊙ , and Sgr A* is generally believed to be powered by gas accretion onto a supermassive black hole. Multifrequency radio observations of the pul...

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Bibliografiset tiedot
Päätekijät: Shenyue Yin, Siming Liu
Aineistotyyppi: Artigo
Kieli:Inglês
Julkaistu: IOP Publishing 2026-01-01
Sarja:The Astrophysical Journal
Aiheet:
Linkit:https://doi.org/10.3847/1538-4357/ae4736
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