Hostname: page-component-78c5997874-8bhkd Total loading time: 0 Render date: 2024-11-14T07:06:55.316Z Has data issue: false hasContentIssue false
  • English
  • Français

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

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

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