{ "id": "2006.08757", "version": "v1", "published": "2020-06-15T20:50:03.000Z", "updated": "2020-06-15T20:50:03.000Z", "title": "Gamma-ray emission revealed at the western edge of SNR G344.7-0.1", "authors": [ "J. Eagle", "S. Marchesi", "M. Ajello", "D. Castro", "A. Vendrasco" ], "comment": "9 pages, 6 figures", "categories": [ "astro-ph.HE" ], "abstract": "We report on the investigation of a very high energy (VHE), Galactic gamma-ray source recently discovered at >50GeV using the Large Area Telescope (LAT) on board the Fermi Gamma-Ray Space Telescope. This object, 2FHL J1703.4-4145, displays a very hard >50GeV spectrum with a photon index ~1.2 in the 2FHL catalog and, as such, is one of the most extreme sources in the 2FHL sub-sample of Galactic objects. A detailed analysis of the available multi-wavelength data shows that this source is located on the western edge of the supernova remnant (SNR) G344.7--0.1, along with extended TeV source, HESS J1702-420. The observations and the spectral energy distribution modeling support a scenario where this gamma-ray source is the byproduct of the interaction between the SNR shock and the dense surrounding medium, with escaping cosmic rays (CRs) diffusing into the dense environment and interacting with a large local cloud, generating the observed TeV emission. If confirmed, an interaction between the SNR CRs and a nearby cloud would make 2FHL J1703.4-4145 another promising candidate for efficient particle acceleration of the 2FHL Galactic sample, following the first candidate from our previous investigation of a likely shock-cloud interaction occurring on the West edge of the Vela SNR.", "revisions": [ { "version": "v1", "updated": "2020-06-15T20:50:03.000Z" } ], "analyses": { "keywords": [ "western edge", "snr g344", "gamma-ray emission", "2fhl j1703", "spectral energy distribution modeling support" ], "note": { "typesetting": "TeX", "pages": 9, "language": "en", "license": "arXiv", "status": "editable" } } }