Prefer a chat interface with context about you and your work?
Observations of the [C <scp>i</scp>] (3<i>P</i>1โ3<i>P</i>0) emission toward the massive star-forming region RCW 38: Further evidence for highly-clumped density distribution of the molecular gas
Abstract We present observations of the 3P1โ3P0 fine-structure line of atomic carbon using the ASTE 10m sub-mm telescope towards RCW 38, the youngest super star cluster in the Milky Way. The detected [C i] emission is compared with the CO J = 1โ0 image cube presented in Fukui et al. โฆ