Internal Physical and Chemical Characteristics of Starless Cores on the Brink of Gravitational Collapse
Using various molecular line and continuum emission criteria, we have selected a sample of six isolated, dense concentrations of molecular gas, i.e., “cores”, which are either starless (L694-2, L429, L1517B, and L1689-SMM16) or contain a protostellar Very Low Luminosity Object (VeLLO) and are cur...
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| Language: | en |
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2014
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| Online Access: | http://hdl.handle.net/1828/5600 |