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Observations of distinct positions in Orion and W3 revealed ripples on theHCN(1-0), HCO^+(1-0) and CO(1-0) line profiles which can be result of emissionof large number of unresolved thermal clumps in the beam that move with randomvelocities. The total number of such clumps are ~(0.4-4) 10^5 for the areaswith linear sizes ~0.1-0.5 pc.

A Search for Small-Scale Clumpiness in Orion and W3 High-Mass Star-Forming Regions