Abstract
The gaseous components studied in HI and OH absorption against the extragalactic radiosources 3C123 and 3C111 are found to be the low-density edges of condensations of a few 100 MThe densest part of one of these condensations has a structure similar to that found in other dark clouds −1 it is fragmented into several cores of a few Mo, with an orbital velocity dispersion ≈ 2 kms . In turn, the extended low-density layer, optically thick in CO (2-1), is not a common feature. It depends on the ambient UV field but the dust temperature in the core may control its existence, even more critically: the lower is the dust temperature, the less massive is the core and the more extended is the envelope around it, for a given total mass in a given external pressure.
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Falgarone, E., Puget, J.L., Evans, N.J., Federman, S.R. (1985). Large and small scale structures of molecular clouds in the taurus perseus complex. In: Serra, G. (eds) Nearby Molecular Clouds. Lecture Notes in Physics, vol 237. Springer, Berlin, Heidelberg. https://doi.org/10.1007/3-540-15991-6_75
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DOI: https://doi.org/10.1007/3-540-15991-6_75
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