Dynamics of different layers traced by [C ii] and CO in bright-rimmed clouds in IC 1396

Y. Okada; R. Güsten; M. Röllig; J. Stutzki; T. Klein; D. Ishihara

doi:10.1051/eas/1575028

All issues

Volume 75-76 (2015)

EAS Publications Series, 75-76 (2015) 163-166

Abstract

Issue		EAS Publications Series Volume 75-76, 2015 Conditions and Impact of Star Formation


Page(s)		163 - 166
Section		Star Formation: Physical and Chemical Conditions, Feedback
DOI		https://doi.org/10.1051/eas/1575028
Published online		20 May 2016

Conditions and Impact of Star Formation
R. Simon, R. Schaaf and J. Stutzki (eds)
EAS Publications Series, 75–76 (2015) 163-166

Dynamics of different layers traced by [C ii] and CO in bright-rimmed clouds in IC 1396

Y. Okada¹, R. Güsten², M. Röllig¹, J. Stutzki¹, T. Klein² and D. Ishihara³

¹ I. Physikalisches Institut der Universität zu Köln, Germany
² Max-Planck-Institut für Radioastronomie, Germany
³ Graduate School of Science, Nagoya University, Japan

e-mail: okada@ph1.uni-koeln.de

Abstract

We mapped 4 bright-rimmed clouds in IC 1396 in the veloci-ty–resolved [C ii] 158 μm emission, and analyzed the dynamics of gas components traced by [C ii] and CO. In all rims the [C ii] emission is not fully reproduced by the CO line profile, indicating a complex origin of the line emission including ablating material.