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Diffuse [CII] Emission in Interstellar Space

Published online by Cambridge University Press:  08 February 2017

H. Okuda ,
H. Shibai ,
T. Nakagawa ,
H. Matsuhara ,
T. Maihara ,
K. Mizutani ,
N. Hiromoto ,
Y. Kobayashi ,
F. J. Low  and
T. Nishimura
H. Okuda
Affiliation:
Institute of Space and Astronautical Science Japan
H. Shibai
Affiliation:
Institute of Space and Astronautical Science Japan
T. Nakagawa
Affiliation:
Institute of Space and Astronautical Science Japan
H. Matsuhara
Affiliation:
Institute of Space and Astronautical Science Japan
T. Maihara
Affiliation:
Kyoto University Japan
K. Mizutani
Affiliation:
Kyoto University Japan
N. Hiromoto
Affiliation:
Communication Research Laboratory Japan
Y. Kobayashi
Affiliation:
Institute of Astronomy University of Tokyo Japan
F. J. Low
Affiliation:
Steward Observatory University of Arizona USA
T. Nishimura
Affiliation:
Steward Observatory University of Arizona USA

Abstract

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An extensive survey of [CII] line emission has been made with a balloon-borne infrared telescope. It has been found that the emission is diffuse and ubiquitously distributed in general interstellar space.

Type
III. Diffuse Galactic Radiation from Dust and Gas: Observations and Models
Information
Symposium - International Astronomical Union , Volume 139: The Galactic and Extragalactic Background Radiation , 1990 , pp. 207 - 209
Copyright
Copyright © Kluwer 1990 

References

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