{ "id": "2207.06698", "version": "v1", "published": "2022-07-14T07:00:49.000Z", "updated": "2022-07-14T07:00:49.000Z", "title": "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" ], "comment": "20 pages, 11 figures, 4 tables, accepted for publication in AJ", "categories": [ "astro-ph.GA" ], "abstract": "We present H I gas kinematics and star formation activities of NGC 6822, a dwarf galaxy located in the Local Group at a distance of ~ 490 kpc. We perform profile decomposition of line-of-sight velocity profiles of the H I data cube (42.4\" x 12.0\" spatial, corresponding to ~ 100 pc; 1.6 km s$^{-1}$ spectral) taken with the Australia Telescope Compact Array (ATCA). For this, we use a new tool, the so-called BAYGAUD which is based on Bayesian analysis techniques, allowing us to decompose a line-of-sight velocity profile into an optimal number of Gaussian components in a quantitative manner. We classify the decomposed H I gas components of NGC 6822 into cool-bulk, warm-bulk, cool-non-bulk and warm-non-bulk motions with respect to their centroid velocities and velocity dispersions. We correlate their gas surface densities with corresponding star formation rate densities derived using both the GALEX far-ultraviolet and WISE 22 $\\mu$m data to examine the resolved Kennicutt-Schmidt (K-S) law for NGC 6822. Of the decomposed H I gas components, the cool-bulk component is likely to better follow the linear extension of the K-S law for molecular hydrogen (H$_2$) at low gas surface densities where H I is not saturated.", "revisions": [ { "version": "v1", "updated": "2022-07-14T07:00:49.000Z" } ], "analyses": { "keywords": [ "gas dynamics", "corresponding star formation rate densities", "low gas surface densities", "gas components", "line-of-sight velocity profile" ], "note": { "typesetting": "TeX", "pages": 20, "language": "en", "license": "arXiv", "status": "editable" } } }