scholarly journals Galactic dynamics feeding the Galactic center

2013 ◽  
Vol 9 (S303) ◽  
pp. 174-176
Author(s):  
Florent Renaud ◽  
Eric Emsellem ◽  
Frédéric Bournaud
Keyword(s):  
Black Hole ◽  
Hierarchical Structure ◽  
Central Region ◽  
Milky Way ◽  
Galactic Center ◽  
Rapid Evolution ◽  
Galactic Dynamics ◽  
Supermassive Black Hole ◽  
The Hierarchical Structure

AbstractWe present the hierarchical structure of the gas and its rapid evolution in the central region of a simulation of the entire Milky Way, run at subparsec resolution. We emphasize the coupling between the kpc-scale dynamics, the molecular ring and the central 5 pc disk feeding the supermassive black hole.

scholarly journals Null Geodesics and Strong Field Gravitational Lensing in a String Cloud Background

2015 ◽  
Vol 2015 ◽  
pp. 1-9 ◽  
Author(s):  
M. Sharif ◽  
Sehrish Iftikhar
Keyword(s):  
Black Hole ◽  
Gravitational Lensing ◽  
Galactic Center ◽  
Deflection Angle ◽  
Orbital Motion ◽  
Strong Field ◽  
Schwarzschild Black Hole ◽  
Field Limit ◽  
Null Geodesics ◽  
Supermassive Black Hole

This paper is devoted to studying two interesting issues of a black hole with string cloud background. Firstly, we investigate null geodesics and find unstable orbital motion of particles. Secondly, we calculate deflection angle in strong field limit. We then find positions, magnifications, and observables of relativistic images for supermassive black hole at the galactic center. We conclude that string parameter highly affects the lensing process and results turn out to be quite different from the Schwarzschild black hole.

scholarly journals The Post-periapsis Evolution of Galactic Center Source G1: The Second Case of a Resolved Tidal Interaction with a Supermassive Black Hole

2017 ◽  
Vol 847 (1) ◽  
pp. 80 ◽  
Author(s):  
G. Witzel ◽  
B. N. Sitarski ◽  
A. M. Ghez ◽  
M. R. Morris ◽  
A. Hees ◽  
...  
Keyword(s):  
Black Hole ◽  
Galactic Center ◽  
Tidal Interaction ◽  
Supermassive Black Hole

scholarly journals A Deep Chandra View of a Candidate Parsec-scale Jet from the Galactic Center Supermassive Black Hole

2019 ◽  
Vol 875 (1) ◽  
pp. 44 ◽  
Author(s):  
Zhenlin Zhu ◽  
Zhiyuan Li ◽  
Mark R. Morris ◽  
Shuo Zhang ◽  
Siming Liu
Keyword(s):  
Black Hole ◽  
Galactic Center ◽  
Supermassive Black Hole

scholarly journals MILKY WAY GLOBULAR CLUSTERS: CLOSE ENCOUNTER RATES WITH EACH OTHER AND WITH THE CENTRAL SUPERMASSIVE BLACK HOLE

REPORTS ◽  
2021 ◽  
Vol 6 (340) ◽  
pp. 94-105
Author(s):  
M.V. Ishchenko ◽  
M.O. Sobolenko ◽  
M.T. Kalambay ◽  
B.T. Shukirgaliyev ◽  
P.P. Berczik
Keyword(s):  
Black Hole ◽  
Globular Clusters ◽  
Milky Way ◽  
Close Encounter ◽  
Encounter Rates ◽  
Supermassive Black Hole

2.9. Microlens mapping of disks in active galactic nuclei

1998 ◽  
Vol 184 ◽  
pp. 75-76 ◽  
Author(s):  
A. Yonehara ◽  
S. Mineshige ◽  
J. Fukue ◽  
M. Umemura ◽  
E.L. Turner
Keyword(s):  
Black Hole ◽  
Active Galactic Nuclei ◽  
Accretion Disk ◽  
Central Region ◽  
Galactic Nuclei ◽  
Direct Information ◽  
Supermassive Black Hole ◽  
Disk Size

Generally, it is believed that there is a supermassive black hole and a surrounding accretion disk in a central region of active galactic nuclei (AGN). However, it is quite difficult to obtain direct information about the center of AGN, because the accretion disk size is far too small to resolve.

scholarly journals Variable Infrared Emission from the Supermassive Black Hole at the Center of the Milky Way

2004 ◽  
Vol 601 (2) ◽  
pp. L159-L162 ◽  
Author(s):  
A. M. Ghez ◽  
S. A. Wright ◽  
K. Matthews ◽  
D. Thompson ◽  
D. Le Mignant ◽  
...  
Keyword(s):  
Black Hole ◽  
Milky Way ◽  
Infrared Emission ◽  
Supermassive Black Hole

scholarly journals 10.2. High proper motions in the vicinity of Sgr A∗: unambiguous evidence for a massive central black hole

1998 ◽  
Vol 184 ◽  
pp. 433-434
Author(s):  
A. M. Ghez ◽  
B. L. Klein ◽  
C. McCabe ◽  
M. Morris ◽  
E. E. Becklin
Keyword(s):  
Black Hole ◽  
Milky Way ◽  
Galactic Center ◽  
Robust Method ◽  
Proper Motions ◽  
Central Black Hole ◽  
Milky Way Galaxy ◽  
The Galaxy ◽  
Sgr A

Although the notion that the Milky Way galaxy contains a supermassive central black hole has been around for more than two decades, it has been difficult to prove that one exists. The challenge is to assess the distribution of matter in the few central parsecs of the Galaxy. Assuming that gravity is the dominant force, the motion of the stars and gas in the vicinity of the putative black hole offers a robust method for accomplishing this task, by revealing the mass interior to the radius of the objects studied. Thus objects located closest to the Galactic Center provide the strongest constraints on the black hole hypothesis.

scholarly journals The Habitability of the Galactic Bulge

Life ◽  
2020 ◽  
Vol 10 (8) ◽  
pp. 132
Author(s):  
Amedeo Balbi ◽  
Maryam Hami ◽  
Andjelka Kovačević
Keyword(s):  
Black Hole ◽  
Milky Way ◽  
Orbital Stability ◽  
Analytical Models ◽  
Radiation Environment ◽  
Habitable Zone ◽  
Central Black Hole ◽  
Supermassive Black Hole ◽  
Star Density ◽  
Rocky Planets

We present a new investigation of the habitability of the Milky Way bulge, that expands previous studies on the Galactic Habitable Zone. We discuss existing knowledge on the abundance of planets in the bulge, metallicity and the possible frequency of rocky planets, orbital stability and encounters, and the possibility of planets around the central supermassive black hole. We focus on two aspects that can present substantial differences with respect to the environment in the disk: (i) the ionizing radiation environment, due to the presence of the central black hole and to the highest rate of supernovae explosions and (ii) the efficiency of putative lithopanspermia mechanism for the diffusion of life between stellar systems. We use analytical models of the star density in the bulge to provide estimates of the rate of catastrophic events and of the diffusion timescales for life over interstellar distances.

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