Comparison of H13CN spectra averaged over pixels where has ≥5σ emission at a) Oph/main; b) Oph/cold; c) Aquila/W40; d) Aquila/Serp. South; e) Aquila/cold; f) NGC 2023; g) NGC 2024; h) NGC 2068; and i) NGC 2071. For Oph/cold, Aquila/cold, and NGC 2023, the H13CN emission is not detected. Thus, we show the spectra averaged over observing area.
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