{ "id": "1203.3234", "version": "v1", "published": "2012-03-14T23:21:37.000Z", "updated": "2012-03-14T23:21:37.000Z", "title": "Fermi-LAT Discovery of GeV Gamma-ray Emission from the Vicinity of SNR W44", "authors": [ "Yasunobu Uchiyama", "Stefan Funk", "Hideaki Katagiri", "Junichiro Katsuta", "Marianne Lemoine-Goumard", "Hiroyasu Tajima", "Takaaki Tanaka", "Diego Torres" ], "comment": "5 pages, accepted for publication in ApJL", "categories": [ "astro-ph.HE" ], "abstract": "We report the detection of GeV gamma-ray emission from the molecular cloud complex that surrounds the supernova remnant (SNR) W44 using the Large Area Telescope (LAT) onboard Fermi. While the previously reported gamma-ray emission from SNR W44 is likely to arise from the dense radio-emitting filaments within the remnant, the gamma-ray emission that appears to come from the surrounding molecular cloud complex can be ascribed to the cosmic rays (CRs) that have escaped from W44. The non-detection of synchrotron radio emission associated with the molecular cloud complex suggests the decay of neutral pi mesons produced in hadronic collisions as the gamma-ray emission mechanism. The total kinetic energy channeled into the escaping CRs is estimated to be (0.3--3)x10^{50} erg, in broad agreement with the conjecture that SNRs are the main sources of Galactic CRs.", "revisions": [ { "version": "v1", "updated": "2012-03-14T23:21:37.000Z" } ], "analyses": { "keywords": [ "gev gamma-ray emission", "snr w44", "fermi-lat discovery", "surrounding molecular cloud complex", "total kinetic energy" ], "tags": [ "journal article" ], "publication": { "doi": "10.1088/2041-8205/749/2/L35", "journal": "The Astrophysical Journal", "year": 2012, "month": "Apr", "volume": 749, "number": 2 }, "note": { "typesetting": "TeX", "pages": 5, "language": "en", "license": "arXiv", "status": "editable", "inspire": 1093922, "adsabs": "2012ApJ...749L..35U" } } }