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Star Formation in the H II Region Sh 2-205: 3D Morphology and Kinematics from Young Stars and Molecular Gas

  • Authors: Yiwei Dong, Chaojie Hao, Ye Xu, Yingjie Li, Zehao Lin, Dejian Liu, Yan Sun, Longhui Yang

Yiwei Dong et al 2026 The Astrophysical Journal 1009 .

  • Provider: AAS Journals

Caption: Figure 8.

CMDs of young stars in each subregion. Black curves show the best-fit isochrones for subregions A–D. Stars fainter than 18 mag (gray shading area) are excluded from the CMD fitting. Subregions E and F are not fitted because of the limited number of young stars. The blue-gray dashed curves indicate the reference theoretical isochrones.

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