{ "id": "2310.01797", "version": "v1", "published": "2023-10-03T04:54:27.000Z", "updated": "2023-10-03T04:54:27.000Z", "title": "On the influence of shock-cloud interactions on the nonthermal X-ray emission from the supernova remnant RCW 86", "authors": [ "Aya Bamba", "Hidetoshi Sano", "Ryo Yamazaki", "Jacco Vink" ], "comment": "10 pages, 27 figures, PASJ, in press", "categories": [ "astro-ph.HE", "hep-ex" ], "abstract": "It is an open issue how the surrounding environment of supernova remnant shocks affect nonthermal X-rays from accelerated electrons, with or without interacting dense material. We have conducted spatially resolved X-ray spectroscopy of the shock-cloud interacting region of RCW 86 with XMM-Newton. It is found that bright soft X-ray filaments surround the dense cloud observed with 12CO and HI emission lines. These filaments are brighter in thermal X-ray emission, and fainter and possibly softer in synchrotron X-rays, compared to those without interaction. Our results show that the shock decelerates due to the interaction with clouds, which results in an enhancements of thermal X-ray emission. This could possibly also explain the softer X-ray synchrotron component, because it implies that those shocks that move through a low density environment, and therefore decelerate much less, can be more efficient accelerators. This is similar to SN 1006 and Tycho, and is in contrast to RX J1713.7-3946. This difference among remnants may be due to the clumpiness of dense material interacting with the shock, which should be examined with future observations.", "revisions": [ { "version": "v1", "updated": "2023-10-03T04:54:27.000Z" } ], "analyses": { "keywords": [ "supernova remnant rcw", "nonthermal x-ray emission", "shocks affect nonthermal x-rays", "remnant shocks affect nonthermal", "shock-cloud interactions" ], "note": { "typesetting": "TeX", "pages": 10, "language": "en", "license": "arXiv", "status": "editable" } } }