ISO-LWS study of Pre-Main Sequence Sources

Details ISO-LWS study of Pre-Main Sequence Sources ISO-LWS study of Pre-Main Sequence Sources

Aug 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999pcim.conf..279s&link_type=abstract

The Physics and Chemistry of the Interstellar Medium, Proceedings of the 3rd Cologne-Zermatt Symposium, held in Zermatt, Septemb

Physics

2

Scientific paper

We present the results obtained with the ISO Long Wavelength Spectrometer on a sample of Pre-MS sources, where several molecular lines of CO, H 2 O and OH have been detected. The analysis of the CO lines indicates that gas temperatures as low as 200 K a re 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.

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