Hot Spots in Sgr A* Accretion Disk: Hydrodynamic Insights

被引：1
作者：
Tito, Elizabeth P. [1 ]
Goncharov, Victor P. [1 ,2 ]
Pavlov, Vadim I. [1 ,3 ]
机构：
[1] Sci Advisory Grp, Pasadena, CA 91125 USA
[2] A M Obukhov Inst Atmospher Phys RAS, Moscow 109017, Russia
[3] Univ Lille, Fac Sci & Technol, F-59000 Lille, France
来源：
UNIVERSE | 2023年 / 9卷 / 01期
关键词：
black hole; accretion disk; hydrodynamics; hot spots; methods; analytical; VORTEX STRUCTURES; FLUID;
D O I：
10.3390/universe9010040
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
The recent image of our galaxy's supermassive black hole Sgr A* derived from the 7 April 2017 data of the Event Horizon Telescope Collaboration shows multiple hot spots in its accretion disk. Using the analytical framework, we demonstrate that the observed hot spots may not be disjoint elements but causally linked components ("petals") of one rotating quasi-stationary macro-structure formed in the thermo-vorticial field within the accretion disk.
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页数：14
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