Search

Image Details

View Article Bookmark & Share

Choose export citation format:

Export Citation
Large resolution
Hi-Resolution Export to PDF PPT Format

Stellar Population and Energy Feedback in the Supergiant Shell LMC 1

  • Authors: Guan-Hong Li, 冠宏 李, Chuan-Jui Li, 傳睿 李, You-Hua Chu, 有花 朱, Po-Sheng Ou, 柏昇 歐, C.-H. Rosie Chen, 昌慧 陳, Konstantin Grishunin, Hsu-Tai Lee, 昫岱 李

Guan-Hong Li et al 2025 The Astronomical Journal 169 .

  • Provider: AAS Journals

Caption: Figure 4.

Upper panel: the G vs. GBP − GRP CMD of stars overlaid with stellar evolutionary tracks and isochrones in Region A. Stars are dereddened by an extinction of AV = 0.35. Middle panel: same as above, but for stars in Region B. Lower panel: same as above, but for stars in Region C.

Other Images in This Article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Image in this article
Copyright and Terms & Conditions

Additional terms of reuse