{ "id": "1202.3125", "version": "v1", "published": "2012-02-14T20:00:10.000Z", "updated": "2012-02-14T20:00:10.000Z", "title": "X-Ray Observations of the Supernova Remnant W28 with Suzaku --- I. Spectral Study of the Recombining Plasma", "authors": [ "Makoto Sawada", "Katsuji Koyama" ], "comment": "Accepted for publication in PASJ; Vol.64 No. 4 (8 pages, 5 figures)", "categories": [ "astro-ph.HE" ], "abstract": "We present the Suzaku results of the mixed-morphology supernova remnant W28. The X-ray spectra of the central region of W28 exhibit many bright emission lines from highly ionized atoms. An optically thin thermal plasma in collisional ionization equilibrium, either of single-temperature or multi-temperature failed to reproduce the data with line-like and bump-like residuals at the Si Lyman$\\alpha$ energy and at 2.4--5.0 keV, respectively. The bumps probably correspond to radiative recombination continua from He-like Si and S. A simple recombining plasma model nicely fit the bump structures, but failed to fit low energy bands. The overall spectra can be fit with a multi-ionization temperature plasma with a common electron temperature. The multi-ionization temperatures are interpreted as elemental difference of ionization and recombination timescales. These results prefer the rarefaction scenario for the origin of the recombining plasma.", "revisions": [ { "version": "v1", "updated": "2012-02-14T20:00:10.000Z" } ], "analyses": { "keywords": [ "spectral study", "x-ray observations", "plasma model nicely fit", "recombining plasma model", "mixed-morphology supernova remnant w28" ], "tags": [ "journal article" ], "publication": { "doi": "10.1093/pasj/64.4.81", "journal": "Publications of the Astronomical Society of Japan", "year": 2012, "month": "Aug", "volume": 64, "pages": 81 }, "note": { "typesetting": "TeX", "pages": 8, "language": "en", "license": "arXiv", "status": "editable", "inspire": 1089063, "adsabs": "2012PASJ...64...81S" } } }