Signatures of UV radiation in low-mass protostars - I. Origin of HCN and CN emission in the Serpens Main region

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Fig. 10

Map of CN 1–0 (colors) and HCN 1–0 (contours) in the Serpens Main. The labels are the same as in Fig. 2. Contour levels start at 8 K km s⁻¹ with steps of 3 K km s⁻¹. The CN emission has been resampled to the beam size of HCN to compare the same emitting regions.

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