Saraceno, P.; Benedettini, M.; di Giorgio, A. M.; Giannini, T.; Nisini, B.; Lorenzetti, D.; Molinari, S.; Pezzuto, S.; Spinoglio, L.; Tommasi, E.; Clegg, P. E.; Correia, J. C.; Griffin, M. J.; Kaufman, M. J.; Leeks, S. J.; White, G.; Caux, E.; Liseau, R. and Smith, H.
(1999).
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| URL: | http://adsabs.harvard.edu/abs/1999pcim.conf..279S |
|---|---|
| Google Scholar: | Look up in Google Scholar |
Abstract
We present the results obtained with the ISO Long Wavelength Spectrometer on a sample of Pre-MS sources, where several molecular lines of CO, H2O and OH have been detected. The analysis of the CO lines indicates that gas temperatures as low as 200 K are consistent with the data. This would be in agreement with the relatively low abundance of water in the gas phase measured in most of the objects.
| Item Type: | Conference Item |
|---|---|
| Copyright Holders: | 1999 Not known |
| Extra Information: | The Physics and Chemistry of the Interstellar Medium, Proceedings of the 3rd Cologne-Zermatt Symposium,
held in Zermatt, September 22-25, 1998, Eds.: V. Ossenkopf, J. Stutzki, and G. Winnewisser, GCA-Verlag Herdecke, ISBN 3-928973-95-9 pp.279-282 |
| Academic Unit/Department: | Science > Physical Sciences |
| Interdisciplinary Research Centre: | Centre for Earth, Planetary, Space and Astronomical Research (CEPSAR) |
| Item ID: | 33300 |
| Depositing User: | Glenn White |
| Date Deposited: | 25 Apr 2012 09:42 |
| Last Modified: | 26 Apr 2012 16:03 |
| URI: | http://oro.open.ac.uk/id/eprint/33300 |
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