Diffuse [CII] Emission in the Galaxy
1996 ◽
Vol 169
◽
pp. 497-498
Keyword(s):
An extensive survey of [C II] line emission at 158 microns using the balloon borne telescope (BICE) has provided a complete map of the emission intensity distribution in the first and the fourth quadrants of the galactic plane (280° < l < 80°, −5° < b < 5°: Okuda et al. 1993). The emission is very extended throughout the galactic plane in which three intensity maxima are seen towards the tangential directions of the Scutum and the Norma arms as well as in the Galactic center region. However the Galactic center maximum is much less prominent compared with the two other distributions, unlike the case of far infrared continuum and CO emissions.
2007 ◽
Vol 16
(12b)
◽
pp. 2399-2405
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Keyword(s):
1980 ◽
Vol 87
◽
pp. 397-404
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Keyword(s):
1988 ◽
Vol 126
◽
pp. 37-48
Keyword(s):
2009 ◽
Vol 5
(S266)
◽
pp. 482-482
Keyword(s):
1987 ◽
Vol 115
◽
pp. 499-499
◽
Keyword(s):
Keyword(s):
1987 ◽
Vol 115
◽
pp. 614-620
Keyword(s):
1989 ◽
Vol 136
◽
pp. 243-263
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Keyword(s):