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Fig. 9

image

Schematic picture for the distribution of dense molecular and ionized gas in a gravitationally unstable, OB cluster-forming molecular clump. Un-shield molecular gas condensations can be externally illuminated and show varieties of ionized features. On the other hand, bright point-like emission sources are expected to be embedded by dense molecular lumps. In low angular resolution observations, this variety of structures will be smeared into an integrated UC Hii region.

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