scholarly journals NuSTARHARD X-RAY SURVEY OF THE GALACTIC CENTER REGION. I. HARD X-RAY MORPHOLOGY AND SPECTROSCOPY OF THE DIFFUSE EMISSION

2015 ◽  
Vol 814 (2) ◽  
pp. 94 ◽  
Author(s):  
Kaya Mori ◽  
Charles J. Hailey ◽  
Roman Krivonos ◽  
Jaesub Hong ◽  
Gabriele Ponti ◽  
...  
2001 ◽  
Vol 27 (8) ◽  
pp. 501-506 ◽  
Author(s):  
A. A. Lutovinov ◽  
S. A. Grebenev ◽  
M. N. Pavlinsky ◽  
R. A. Sunyaev
Keyword(s):  
X Ray ◽  

2002 ◽  
Vol 565 (2) ◽  
pp. 1017-1021 ◽  
Author(s):  
Atsushi Senda ◽  
Hiroshi Murakami ◽  
Katsuji Koyama
Keyword(s):  
X Ray ◽  

1985 ◽  
Vol 290 ◽  
pp. 557 ◽  
Author(s):  
F. K. Knight ◽  
W. N., III Johnson ◽  
J. D. Kurfess ◽  
M. S. Strickman

1991 ◽  
Author(s):  
A. Bazzano ◽  
C. La Padula ◽  
P. Ubertini ◽  
R. K. Sood
Keyword(s):  
X Ray ◽  

1998 ◽  
Vol 184 ◽  
pp. 443-444 ◽  
Author(s):  
Masaaki Sakano ◽  
Mamiko Nishiuchi ◽  
Yoshitomo Maeda ◽  
Katsuji Koyama ◽  
Jun Yokogawa

We report the column density distribution to the Galactic Center region using the X-ray binary observations with the X-ray satellite ASCA, and demonstrate a new method of the total mass determination near the Galactic Center. The column densities are given by a simple form as a function of the angular distance from the Galactic Plane. Assuming a disklike mass distribution of 500 pc radius, we estimate the total mass to be ~ 6 × 107M⊙.


1984 ◽  
Vol 81 ◽  
pp. 219-221
Author(s):  
John A. Nousek ◽  
Gordon P. Garmire ◽  
George Weaver

Maps of the diffuse soft X-ray background intensity are presented, spanning four energy intervals. The lowest energy interval (0.18-0.56 keV) is dominated by local emission, while the next two intervals (0.56-1.0 keV and 1.0-1.4 keV) reveal more distant and more sharply defined structures. Enlarged maps of several of these structures are presented, including the North Polar Spur, the Galactic Center region and the Eridanus Loop.


2004 ◽  
Vol 153 (1) ◽  
pp. 395-395 ◽  
Author(s):  
Christopher L. Martin ◽  
Wilfred M. Walsh ◽  
Kecheng Xiao ◽  
Adair P. Lane ◽  
Christopher K. Walker ◽  
...  

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