{ "id": "2212.00097", "version": "v1", "published": "2022-11-30T20:08:58.000Z", "updated": "2022-11-30T20:08:58.000Z", "title": "High-Resolution Spectra of Supernova Remnants in M83", "authors": [ "P. Frank Winkler", "Knox S. Long", "William P. Blair", "Sean D. Points" ], "comment": "39 pages, including 9 figures (some with multiple sub-figures) and 6 tables", "categories": [ "astro-ph.GA", "astro-ph.HE", "astro-ph.SR" ], "abstract": "In order to better characterize the rich supernova remnant (SNR) population of M83 (NGC 5236), we have obtained high-resolution (about 85 km/s) spectra of 119 of the SNRs and SNR candidates in M83 with Gemini/GMOS, as well as new spectra of the young SNRs B12-174a and SN1957D. Most of the SNRs and SNR candidates have [S II]:H{\\alpha} ratios that exceed 0.4. Combining these results with earlier studies we have carried out with MUSE and at lower spectroscopic resolution with GMOS, we have confirmed a total of 238 emission nebulae to be SNRs on the basis of their [S II]:H{\\alpha} ratios, about half of which have emission lines that show velocity broadening greater than 100 km/s, providing a kinematic confirmation that they are SNRs and not H II regions. Looking at the entire sample, we find a strong correlation between velocity widths and the line ratios of [O I]{\\lambda}6300:H{\\alpha}, [N II]{\\lambda}6584:H{\\alpha} and [S II]{\\lambda}{\\lambda}6716,6731:H{\\alpha}. The density-sensitive [S II]{\\lambda}6716:{\\lambda}6731 line ratio is strongly correlated with SNR diameter, but not with the velocity width. We discuss these results in the context of previously published shock models.", "revisions": [ { "version": "v1", "updated": "2022-11-30T20:08:58.000Z" } ], "analyses": { "keywords": [ "high-resolution spectra", "snr candidates", "line ratio", "velocity width", "young snrs b12-174a" ], "note": { "typesetting": "TeX", "pages": 39, "language": "en", "license": "arXiv", "status": "editable" } } }