White, Glenn J. and Padman, Rachael
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At the interface between an HII region and a molecular cloud, lies a neutral gas layer which is subject to both an intense radiation field, and to shocks arising from the expansion of the ionisation front of the HII region. The gas in these regions is highly excited, hot, and may be fairly dense. We present the first high resolution images of atomic carbon towards a sample of ionisation front sources. This study has relevance to our understanding of shock induced star formation, the formation and destruction of molecular species under extreme conditions, shock processes in the ISM, and the energy balance in molecular clouds.
|Item Type:||Conference Item|
|Copyright Holders:||1992 IAU|
|Extra Information:||Astrochemistry of Cosmic Phenomena:
Proceedings of the 150th Symposium of the International Astronomical Union,
held at Campos do Jordao, Sao Paulo, Brazil, August 5-9, 1991.
Edited by P. D. Singh.
International Astronomical Union. Symposium no. 150,
Kluwer Academic Publishers, Dordrecht, 1992.,
|Academic Unit/Department:||Faculty of Science, Technology, Engineering and Mathematics (STEM) > Physical Sciences
Faculty of Science, Technology, Engineering and Mathematics (STEM)
|Interdisciplinary Research Centre:||Centre for Earth, Planetary, Space and Astronomical Research (CEPSAR)|
|Depositing User:||G. J. White|
|Date Deposited:||30 May 2012 14:59|
|Last Modified:||05 Oct 2016 07:06|
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