Coherence in Dense Cores. Ii. the Transition to Coherence

@inproceedings{GV1998CoherenceID,
  title={Coherence in Dense Cores. Ii. the Transition to Coherence},
  author={A. G.V.},
  year={1998}
}
After studying how line width depends on spatial scale in low-mass star-forming regions, we propose that ““ dense cores ÏÏ & Benson represent an inner scale of a self-similar process that charac(Myers 1983) terizes larger scale molecular clouds. In the process of coming to this conclusion, we deÐne four distinct types of line widthÈsize relation which have power-law slopes and as follows : Type 1Èmultitracer, multicloud (*vP Rai), a1, a2, a3, a4, intercomparison ; Type 2Èsingle-tracer… CONTINUE READING
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