{ "id": "1201.6031", "version": "v1", "published": "2012-01-29T11:56:46.000Z", "updated": "2012-01-29T11:56:46.000Z", "title": "Interstellar gas within $\\sim 10$ pc of Sgr A$^*$", "authors": [ "Katia Ferriere" ], "comment": "21 pages, 7 figures", "categories": [ "astro-ph.GA" ], "abstract": "We seek to obtain a coherent and realistic three-dimensional picture of the interstellar gas out to about 10 pc of the dynamical center of our Galaxy, which is supposed to be at Sgr A$^*$. We review the existing observational studies on the different gaseous components that have been identified near Sgr A$^*$, and retain all the information relating to their spatial configuration and/or physical state. Based on the collected information, we propose a three-dimensional representation of the interstellar gas, which describes each component in terms of both its precise location and morphology and its thermodynamic properties. The interstellar gas near Sgr A$^*$ can represented by five basic components, which are, by order of increasing size: (1) a central cavity with roughly equal amounts of warm ionized and atomic gases, (2) a ring of mainly molecular gas, (3) a supernova remnant filled with hot ionized gas, (4) a radio halo of warm ionized gas and relativistic particles, and (5) a belt of massive molecular clouds. While the halo gas fills $\\approx 80%$ of the studied volume, the molecular components enclose $\\approx 98%$ of the interstellar mass.", "revisions": [ { "version": "v1", "updated": "2012-01-29T11:56:46.000Z" } ], "analyses": { "keywords": [ "interstellar gas", "realistic three-dimensional picture", "ionized gas", "halo gas fills", "molecular components enclose" ], "tags": [ "journal article" ], "publication": { "doi": "10.1051/0004-6361/201117181", "journal": "Astronomy and Astrophysics", "year": 2012, "month": "Apr", "volume": 540 }, "note": { "typesetting": "TeX", "pages": 21, "language": "en", "license": "arXiv", "status": "editable", "inspire": 1086653, "adsabs": "2012A&A...540A..50F" } } }