scholarly journals AKARI Far-Infrared Spectroscopic Observations of the Galactic Center Region

2009 ◽  
Vol 61 (3) ◽  
pp. 511-520 ◽  
Author(s):  
Akiko Yasuda ◽  
Hidehiro Kaneda ◽  
Takao Nakagawa ◽  
Yoko Okada ◽  
Mitsunobu Kawada ◽  
...  
Keyword(s):  
Galactic Center ◽  
Far Infrared ◽  
Spectroscopic Observations ◽  
Center Region ◽  
Infrared Spectroscopic

scholarly journals Far-infrared spectroscopic observations of the Galactic center region

2008 ◽  
Vol 480 (1) ◽  
pp. 157-166 ◽  
Author(s):  
A. Yasuda ◽  
T. Nakagawa ◽  
M. Spaans ◽  
Y. Okada ◽  
H. Kaneda
Keyword(s):  
Galactic Center ◽  
Far Infrared ◽  
Spectroscopic Observations ◽  
Center Region ◽  
Infrared Spectroscopic

Liquid-helium-cooled Fabry-Perot spectrometer and the frequency switching method for far-infrared spectroscopic observations

1990 ◽  
Author(s):  
Takao Nakagawa ◽  
Haruyuki Okuda ◽  
Hiroshi Shibai ◽  
Hideo Matsuhara ◽  
Yukiyasu Kobayashi ◽  
...  
Keyword(s):  
Liquid Helium ◽  
Far Infrared ◽  
Spectroscopic Observations ◽  
Fabry Perot ◽  
Infrared Spectroscopic ◽  
Switching Method

Far Infrared Spectral Observations of the Galactic Center Region from the Gerard P. Kuiper Airborne Observatory

1977 ◽  
pp. 126-126
Author(s):  
L. J. Caroff ◽  
E. F. Erickson ◽  
D. Goorvitch ◽  
J. D. Scargle ◽  
J. P. Simpson ◽  
...  
Keyword(s):  
Galactic Center ◽  
Far Infrared ◽  
Center Region ◽  
Infrared Spectral

scholarly journals Observation of Diffuse CII Emission in the Galactic Center Region

1989 ◽  
Vol 136 ◽  
pp. 145-149
Author(s):  
H. Okuda ◽  
H. Shibai ◽  
T. Nakagawa ◽  
T. Matsuhara ◽  
T. Maihara ◽  
...  
Keyword(s):  
Galactic Center ◽  
Line Emission ◽  
Wide Area ◽  
Strong Emission ◽  
Spectroscopic Observations ◽  
Center Region ◽  
Fabry Perot ◽  
Galactic Longitude

Spectroscopic observations of CII line emission at 157.7 μm have been made of the Galactic Center region with a Fabry-Perot spectrometer onboard a balloon telescope. Strong emission has been detected ubiquitously in a wide area extending between ± 0.7° in galactic longitude. A ring-like structure is suggested from the double lobed distribution of the emission around the Galactic Center.

Airborne far-infrared observations of the galactic center region

1977 ◽  
Vol 216 ◽  
pp. 277 ◽  
Author(s):  
I. Gatley ◽  
E. E. Becklin ◽  
C. G. Wynn-Williams ◽  
M. W. Werner
Keyword(s):  
Galactic Center ◽  
Far Infrared ◽  
Infrared Observations ◽  
Center Region

Far-Infrared Observation of the Galactic-Center Region at 100 Microns

1969 ◽  
Vol 155 ◽  
pp. L9 ◽  
Author(s):  
William F. Hoffmann ◽  
Carl L. Frederick
Keyword(s):  
Galactic Center ◽  
Far Infrared ◽  
Infrared Observation ◽  
Center Region

Balloon-borne far-infrared spectrophotometry of the galactic center region

1985 ◽  
Vol 5 (3) ◽  
pp. 7-10 ◽  
Author(s):  
S. Drapatz ◽  
L. Haser ◽  
R. Hofmann ◽  
N. Oda ◽  
R. Wilczek
Keyword(s):  
Galactic Center ◽  
Far Infrared ◽  
Infrared Spectrophotometry ◽  
Center Region

Airborne far-infrared spectroscopic observations of W51 and W49

1979 ◽  
Vol 234 ◽  
pp. 897 ◽  
Author(s):  
T. Herter ◽  
J. G. Duthie ◽  
J. L. Pipher ◽  
M. P. Savedoff
Keyword(s):  
Far Infrared ◽  
Spectroscopic Observations ◽  
Infrared Spectroscopic

scholarly journals Gamma-Ray Imaging of the Galactic Center Region

1989 ◽  
Vol 136 ◽  
pp. 581-585
Author(s):  
W. R. Cook ◽  
D. M. Palmer ◽  
T. A. Prince ◽  
S. M. Schindler ◽  
C. H. Starr ◽  
...  
Keyword(s):  
Gamma Ray ◽  
Galactic Center ◽  
Coded Aperture ◽  
Center Region ◽  
Gamma Ray Imaging ◽  
The Galaxy ◽  
Γ Ray ◽  
Luminous Objects

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.

scholarly journals Discovery of K-Shell Emission Lines of Neutral Atoms in the Galactic Center Region

2010 ◽  
Vol 62 (2) ◽  
pp. 423-429 ◽  
Author(s):  
Masayoshi Nobukawa ◽  
Katsuji Koyama ◽  
Takeshi Go Tsuru ◽  
Syukyo G. Ryu ◽  
Vincent Tatischeff
Keyword(s):  
Galactic Center ◽  
Emission Lines ◽  
Neutral Atoms ◽  
Center Region
Sign in / Sign up

Export Citation Format

Share Document