scholarly journals Deformed black hole in Sagittarius A

2021 ◽  
Vol 103 (12) ◽  
Author(s):  
T. Anson ◽  
E. Babichev ◽  
C. Charmousis
Keyword(s):  
2014 ◽  
Vol 10 (S312) ◽  
pp. 274-281
Author(s):  
Rainer Schödel

AbstractBecause of its nearness to Earth, the centre of the Milky Way is the only galaxy nucleus in which we can study the characteristics, distribution, kinematics, and dynamics of the stars on milli-parsec scales. We have accurate and precise measurements of the Galactic centre's central black hole, Sagittarius A*, and can study its interaction with the surrounding nuclear star cluster in detail. This contribution aims at providing a concise overview of our current knowledge about the Milky Way's central black hole and nuclear star cluster, at highlighting the observational challenges and limitations, and at discussing some of the current key areas of investigation.


2018 ◽  
Vol 478 (4) ◽  
pp. 5209-5229 ◽  
Author(s):  
Andrew Chael ◽  
Michael Rowan ◽  
Ramesh Narayan ◽  
Michael Johnson ◽  
Lorenzo Sironi

2011 ◽  
Vol 63 (5) ◽  
pp. 1093-1116 ◽  
Author(s):  
Makoto Miyoshi ◽  
Zhi-Qiang Shen ◽  
Tomoaki Oyama ◽  
Rohta Takahashi ◽  
Yoshiaki Kato

2016 ◽  
Vol 25 (12) ◽  
pp. 1644021 ◽  
Author(s):  
Hal M. Haggard ◽  
Carlo Rovelli

Recent VLBI observations have resolved Sagittarius A* at horizon scales. The event horizon telescope is expected to provide increasingly good images of the region around the Schwarzschild radius [Formula: see text] of Sgr A* soon. A number of authors have recently pointed out the possibility that nonperturbative quantum gravitational phenomena could affect the space surrounding a black hole. Here, we point out that the existence of a region around [Formula: see text], where these effects should be maximal.


Sign in / Sign up

Export Citation Format

Share Document