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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 6.

The mass distribution for the velocity dispersions. The bin width of the histogram is 0.8 km s−1. Green, red, and blue bars indicate the H I mass distribution derived from MOMENT0, SGfit, and OptGfit (BAYGAUD) integrated flux density maps, respectively.

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