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A New Cloud–Cloud Collision Source N68 toward the G35 Molecular Cloud Complex

  • Authors: En Chen, Xi Chen

En Chen and Xi Chen 2026 The Astrophysical Journal 1001 .

  • Provider: AAS Journals

Caption: Figure 5.

(a) Column density extracted from PPMAP. The white dotted contours indicate the 13CO moment 0 map integrated from 47 to 64 km s−1 with contour levels from 16 (3σ) to 56 K km s−1 in steps of 8 K km s−1 . The red open circles and black open triangles indicate the Class I and Class II YSOs identified in Section 3.2, respectively. The black squares indicate the ATLASGAL clumps. (b) Column density estimated from 13CO. The massive star formation signatures (6.7 GHz masers, MSX sources, and H II regions) are drawn in the same manner as in Figure 2. (c) Dust temperature extracted from PPMAP. (d) FUV field. The contour levels at G0 =  300, 500, 1000, and 3000 are drawn. The dashed lines in panels (b) and (d) divide the R1 region into four main clouds, namely, Clouds 1–4.

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