Looking for evidence of high-mass star formation at core scale in a massive molecular clump

Open Access

Fig. 9

CH₃CN J = 13–12 moment 1 map (from K = 4 projection). The black contours represent the continuum emission at 340 GHz with levels at 1, 10, 30, 60, 90, and 140 mJy beam⁻¹. The dashed black line indicates the direction of the molecular outflow related to core C1. The beams are indicated in the bottom left corner.

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