{ "id": "2406.00903", "version": "v1", "published": "2024-06-03T00:04:59.000Z", "updated": "2024-06-03T00:04:59.000Z", "title": "Revisiting Gamma-Ray Emission of the Supernova Remnant RCW 103", "authors": [ "Yi Xing", "Zhongxiang Wang", "Dong Zheng" ], "comment": "7 pages, 4 figures, 2 tables, submitted to ApJ", "categories": [ "astro-ph.HE" ], "abstract": "We analyze more than 15 years of the \\gr\\ data, obtained with the Large Area Telescope (LAT) onboard {\\it the Fermi Gamma-ray Space Telescope (Fermi)}, for the region of the young supernova remnant (SNR) RCW~103, since the nearby source 4FGL J1616.2$-$5054e, counterpart to HESS~J1616$-$518 and $\\simeq$13\\,arcmin away from the SNR, is determined to be extended in the more recent Fermi-LAT source catalog. Different templates for 4FGL J1616.2$-$5054e and RCW~103 are tested, and we find that a point source with a power-law (PL) spectrum at the southern limb of the SNR best describes the detected gamma-ray emission. The photon index of the PL emission is $\\Gamma\\simeq 2.31$, softer than the previously reported $\\Gamma\\simeq 2.0$ when the counterpart to HESS~J1616$-$518 was considered to be a point source (which likely caused mis-identification of extended emission at RCW~103). In order to produce the \\gr\\ emission in a hadronic scenario, we estimate that protons with an index$\\sim$2.4 PL energy distribution are needed. These results fit with those from multi-wavelength observations that have indicated the remnant at the southern limb is interacting with a molecular cloud.", "revisions": [ { "version": "v1", "updated": "2024-06-03T00:04:59.000Z" } ], "analyses": { "keywords": [ "supernova remnant rcw", "revisiting gamma-ray emission", "fermi gamma-ray space telescope", "nearby source 4fgl j1616", "point source" ], "note": { "typesetting": "TeX", "pages": 7, "language": "en", "license": "arXiv", "status": "editable" } } }