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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 7.

The result of the model tilted-ring fit derived in Weldrake et al. (2003). The left panels show the radial model position angle (P.A.), inclination (i), and model reference velocity (V model). The right panel describes the model velocity field using the radial parameters in the left panels. The solid contours are in steps of 10 km s−1 from −110 to 0 km s−1.