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| | FIR mapping of bok globules CB202, CB220 and CB236(L1166) with ISOPHOT (Site not responding. Last check: 2007-11-02) |
 | | Therefore, due to their optical appearance, Bok globules are of great interest in the study of star formation, as they are possible candidates for harboring such objects. |
 | | The results from a preliminary analysis of these data, based on single short scans across the globules at 100 and 200 microns, has already been presented (Russell et al, 1998, Star Formation with ISO, p214), but was restricted to an investigation of the morphology of the FIR emission. |
 | | The initial single short scans across these globules have yielded detections of cold dust at 200 microns, but, due to the limited field of view, it has not been possible to determine the total flux from these small extended sources. |
| isowww.estec.esa.nl /meetings/paris/Paris_abstracts/node135.html (384 words) |
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