Fig. 13
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(a) Luminosity-mass ratio of the clumps arranged in the proposed evolutionary sequence. (b) Luminosity-mass vs. temperature determined from CO, submillimeter, and CH3CCH emissions. (c) Luminosity-mass vs. column density determined from CO and submillimeter emissions. (d) 870 µm peak flux density vs. CCH integrated intensity. (e) Column density plot of H13CO+ vs. CCH. (f) Full width at half maximum plot of H13CO+(3−2) vs. CCH(35/2.3–23/2.2).
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