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Gillespie, A. R.; White, G. J. and Watt, G. D.
(1979).
DOI: https://doi.org/10.1093/mnras/186.2.383
Abstract
CO observations at 115 GHz are presented for three southern HII regions, RCW 38, RCW 122 and G 316.8-0.1. All three are shown to have large molecular clouds associated with them containing CO peaks in addition to the CO associated with the main optical-HII/radio-continuum sources These are also interpreted as sites of star formation.