Search

Image Details

View Article Bookmark & Share

Choose export citation format:

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

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.

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
Image in this article
Image in this article
Image in this article
Image in this article
Copyright and Terms & Conditions

Additional terms of reuse