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Contribution of line emission to the IRAS measurements: NGC 6853

Published online by Cambridge University Press:  04 August 2017

C. Y. Zhang ,
A. Leene ,
S. R. Pottasch  and
J. E. Mo
C. Y. Zhang
Affiliation:
1. Kapteyn Astronomical Institute, P.O. Box 800, 9700 AV Groningen, Holland 2. Purple Mountain Observatory, Academia Sinica, Nanjing, China
A. Leene
Affiliation:
1. Kapteyn Astronomical Institute, P.O. Box 800, 9700 AV Groningen, Holland
S. R. Pottasch
Affiliation:
1. Kapteyn Astronomical Institute, P.O. Box 800, 9700 AV Groningen, Holland
J. E. Mo
Affiliation:
1. Kapteyn Astronomical Institute, P.O. Box 800, 9700 AV Groningen, Holland 2. Purple Mountain Observatory, Academia Sinica, Nanjing, China

Abstract

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The contribution from the line emission of ions to the radiation at four IRAS bands has been estimated. The dust grains are likely to be mixed with ionized gas.

Type
Circumstellar Shells and Envelopes
Information
Symposium - International Astronomical Union , Volume 122: Circumstellar Matter , 1987 , pp. 219 - 220
Copyright
Copyright © Reidel 1987 

References

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