Precessing jets in Sagittarius A - Gas dynamics in the central parsec of the galaxy

1982 ◽  
Vol 262 ◽  
pp. 110 ◽  
Author(s):  
R. L. Brown
2003 ◽  
Vol 591 (2) ◽  
pp. 891-915 ◽  
Author(s):  
F. K. Baganoff ◽  
Y. Maeda ◽  
M. Morris ◽  
M. W. Bautz ◽  
W. N. Brandt ◽  
...  

2019 ◽  
Vol 885 (2) ◽  
pp. 142 ◽  
Author(s):  
Kaya Mori ◽  
Charles J. Hailey ◽  
Shifra Mandel ◽  
Yve E. Schutt ◽  
Matteo Bachetti ◽  
...  
Keyword(s):  
X Ray ◽  

2006 ◽  
Vol 2 (14) ◽  
pp. 207-207
Author(s):  
Fabrice Martins ◽  
Reinhard Genzel ◽  
Frank Eisenhauer ◽  
Thibaut Paumard ◽  
Thomas Ott ◽  
...  

AbstractThe stellar and wind properties of the new population of massive stars in the central parsec of the Galaxy are derived through quantitative analysis with atmosphere models.


1994 ◽  
Vol 158 ◽  
pp. 379-381
Author(s):  
A. Eckart ◽  
R. Genzel ◽  
R. Hofmann ◽  
B.J. Sams ◽  
L.E. Tacconi-Garman

We present deep 1.6 and 2.2 μm images of the central parsec of the Galaxy at a resolution of 0.15″. Most of the flux in earlier seeing limited images comes from about 340 unresolved stellar sources with K≤14. The IRS 16 and 13 complexes are resolved into about two dozen and half a dozen sources, a number of which are probably luminous hot stars. We confirm the presence of a blue near infrared object (K≈13) at the position of the compact radio source Sgr A∗. The spatial centroid of the source number distribution is consistent with the position of Sgr A∗ but not with a position in the IRS 16 complex. The stellar surface density in the central 10″ is very well fitted by an isothermal cluster model with a well defined core radius. The derived core radius of all 340 sources is 0.15±0.05 pc. The central stellar density is a few times 107 M⊙ pc−3. Buildup of massive stars by merging of lower mass stars and collisional disruption of giant atmospheres are very probable processes in the central 0.2 pc.


1970 ◽  
Vol 39 ◽  
pp. 22-50 ◽  
Author(s):  
Harold F. Weaver

The task assigned for this review is to discuss structural features of the Galaxy as they may involve or relate to gas dynamics. Since a topic of such great breadth would permit discussion of essentially any aspect of the Galaxy, we shall narrow the view and direct attention primarily towards the larger-scale features of the system. In particular, effort will be made to place emphasis on those areas of the subject in which problems of interpretation exist and in which new theoretical models are needed.


2010 ◽  
Vol 723 (2) ◽  
pp. 1097-1109 ◽  
Author(s):  
Jun-Hui Zhao ◽  
Ray Blundell ◽  
James M. Moran ◽  
Dennis Downes ◽  
Karl F. Schuster ◽  
...  

2018 ◽  
Vol 476 (1) ◽  
pp. 235-245 ◽  
Author(s):  
P F Roche ◽  
E Lopez-Rodriguez ◽  
C M Telesco ◽  
R Schödel ◽  
C Packham

1996 ◽  
Vol 459 ◽  
pp. 627 ◽  
Author(s):  
D. A. Roberts ◽  
F. Yusef-Zadeh ◽  
W. M. Goss
Keyword(s):  

1996 ◽  
Vol 467 ◽  
pp. 645 ◽  
Author(s):  
M. Tamura ◽  
M. W. Werner ◽  
E. E. Becklin ◽  
E. S. Phinney
Keyword(s):  

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