{ "id": "1008.1840", "version": "v2", "published": "2010-08-11T06:42:32.000Z", "updated": "2010-09-30T05:28:58.000Z", "title": "Gamma-ray Emission from Crushed Clouds in Supernova Remnants", "authors": [ "Yasunobu Uchiyama", "Roger Blandford", "Stefan Funk", "Hiroyasu Tajima", "Takaaki Tanaka" ], "comment": "5 pages, 2 figures, minor modifications made in Introduction and Discussion, accepted for publication in ApJL", "categories": [ "astro-ph.HE" ], "abstract": "It is shown that the radio and gamma-ray emission observed from newly-found \"GeV-bright\" supernova remnants (SNRs) can be explained by a model, in which a shocked cloud and shock-accelerated cosmic rays (CRs) frozen in it are simultaneously compressed by the supernova blastwave as a result of formation of a radiative cloud shock. Simple reacceleration of pre-existing CRs is generally sufficient to power the observed gamma-ray emission through the decays of neutral pions produced in hadronic interactions between high-energy protons (nuclei) and gas in the compressed-cloud layer. This model provides a natural account of the observed synchrotron radiation in SNRs W51C, W44 and IC 443 with flat radio spectral index, which can be ascribed to a combination of secondary and reaccelerated electrons and positrons.", "revisions": [ { "version": "v2", "updated": "2010-09-30T05:28:58.000Z" } ], "analyses": { "keywords": [ "gamma-ray emission", "supernova remnants", "crushed clouds", "flat radio spectral index", "shock-accelerated cosmic rays" ], "tags": [ "journal article" ], "publication": { "doi": "10.1088/2041-8205/723/1/L122", "journal": "The Astrophysical Journal", "year": 2010, "month": "Nov", "volume": 723, "number": 1 }, "note": { "typesetting": "TeX", "pages": 5, "language": "en", "license": "arXiv", "status": "editable", "inspire": 864966, "adsabs": "2010ApJ...723L.122U" } } }