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An extensive study of interstellar matter in the IC 1396 region using several molecular lines and transitions of CO and far-infrared maps from IRAS

Published online by Cambridge University Press:  03 August 2017

H. Weikard ,
K. Sugitani ,
G. Duvert  and
M. Miller
H. Weikard
Affiliation:
Observatoire de Grenoble, B.P. 53 X, 38041 Grenoble CEDEX, France I. Physikalisches Institut der Universität zu Köln, Zülpicher Straße 77, 5000 Köln, FRG
K. Sugitani
Affiliation:
Department of Astrophysics, Nagoya University, Chikusa-ku, Nagoya 464, Japan I. Physikalisches Institut der Universität zu Köln, Zülpicher Straße 77, 5000 Köln, FRG
G. Duvert
Affiliation:
Observatoire de Grenoble, B.P. 53 X, 38041 Grenoble CEDEX, France
M. Miller
Affiliation:
I. Physikalisches Institut der Universität zu Köln, Zülpicher Straße 77, 5000 Köln, FRG

Abstract

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IC 1396 is an H II region in Cepheus excited by the massive 06.5 star HD 206267. The distance is about 750 pc. The region exhibits a number of bright-rimmed molecular clouds in which outflows have been detected (Sugitani et al. 1989, Duvert et al. 1990).

Type
Poster Sessions
Information
Symposium - International Astronomical Union , Volume 147: Fragmentation of Molecular Clouds and Star Formation , 1991 , pp. 513 - 514
Copyright
Copyright © Kluwer 1991 

References

Duvert, G., Cernicharo, J., Bachiller, R., and Gómez-González, J.: Astron. Astrophys. 233, 190 Google Scholar
Pottasch, S.: Bull. Astron. Inst. Netherlands 13, 77 (1956) (1990) Google Scholar
Sugitani, K., Fukui, Y., Mizuno, A., and Ohashi, N.: Astrophys. J. 342, L87 (1989)CrossRefGoogle Scholar