scholarly journals HCN J = 4–3, HNC J = 1–0, H13CN J = 1–0, and HC3N J = 10–9 Maps of Galactic Center Region. II. Physical Properties of Dense-gas Clumps and Probability of Star Formation

2020 ◽  
Vol 903 (2) ◽  
pp. 111
Author(s):  
Kunihiko Tanaka ◽  
Makoto Nagai ◽  
Kazuhisa Kamegai ◽  
Takahiro Iino ◽  
Takeshi Sakai
2016 ◽  
Vol 825 (2) ◽  
pp. 132 ◽  
Author(s):  
JaeSub Hong ◽  
Kaya Mori ◽  
Charles J. Hailey ◽  
Melania Nynka ◽  
Shuo Zhang ◽  
...  

1998 ◽  
Vol 179 ◽  
pp. 189-190
Author(s):  
T. Oka ◽  
T. Hasegawa ◽  
F. Sato ◽  
H. Yamasaki ◽  
M. Tsuboi ◽  
...  

Molecular gas in the Galactic center region is spatially and kinematically complex, and its physical conditions are distinctively different from those of molecular gas in the Galactic disk (e.g., Morris 1996). Relative paucity of current star formation activity, despite the abundance of dense molecular gas in this region, is one of the problem at issue.


2009 ◽  
Vol 692 (1) ◽  
pp. 47-60 ◽  
Author(s):  
Karl M. Menten ◽  
Robert W. Wilson ◽  
Silvia Leurini ◽  
Peter Schilke

2014 ◽  
Vol 563 ◽  
pp. A68 ◽  
Author(s):  
E. T. Chambers ◽  
F. Yusef-Zadeh ◽  
J. Ott

1989 ◽  
Vol 136 ◽  
pp. 581-585
Author(s):  
W. R. Cook ◽  
D. M. Palmer ◽  
T. A. Prince ◽  
S. M. Schindler ◽  
C. H. Starr ◽  
...  

The Caltech imaging γ-ray telescope was launched by balloon from Alice Springs, NT, Australia and performed observations of the galactic center during the period 12.62 to 13.00 April 1988 UT. The first coded-aperture images of the galactic center region at energies above 30 keV show a single strong γ-ray source which is located 0.7±0.1° from the galactic nucleus and is tentatively identified as 1E1740.7-2942. If the source is at the distance of the galactic center, it is one of the most luminous objects in the galaxy at energies from 35 to 200 keV.


2014 ◽  
Vol 564 ◽  
pp. A106 ◽  
Author(s):  
P. Tremblin ◽  
N. Schneider ◽  
V. Minier ◽  
P. Didelon ◽  
T. Hill ◽  
...  

2010 ◽  
Vol 62 (2) ◽  
pp. 423-429 ◽  
Author(s):  
Masayoshi Nobukawa ◽  
Katsuji Koyama ◽  
Takeshi Go Tsuru ◽  
Syukyo G. Ryu ◽  
Vincent Tatischeff

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