Abstract
We have observed CS and SO emission from a number of dark cloud cores in Taurus, and present maps of CS, SO and their isotopomers towards three of them. On the basis of these maps, there is some evidence for chemical differences between the cores, which may make some of them better candidates for the detection of molecular oxygen by the ODIN satellite.
Original language | English |
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Title of host publication | Chemistry as a Diagnostic of Star Formation |
Subtitle of host publication | Proceedings of the Conference Held in Waterloo, Canada, August 21-23, 2002 |
Editors | Charles Curry, Michel Fich |
Place of Publication | Canada |
Publisher | NRC Research Press |
Pages | 431-433 |
Number of pages | 3 |
ISBN (Print) | 0660190893 |
Publication status | Published - 2003 |
Externally published | Yes |