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Gas Dynamics and Star Formation in NGC 6822

  • Authors: Hye-Jin Park, Se-Heon Oh, Jing Wang, Yun Zheng, Hong-Xin Zhang, W. J. G. De Blok

Hye-Jin Park et al 2022 The Astronomical Journal 164 .

  • Provider: AAS Journals

Caption: Figure 2.

The GALEX FUV (a) and WISE-W4 band (b) images of NGC 6822 degraded to 48.0″ × 48.0″. The contour presents H I gas distribution where its column density is higher than 3.6 × 1019 cm−2.

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