{ "id": "1404.1841", "version": "v1", "published": "2014-04-07T16:31:07.000Z", "updated": "2014-04-07T16:31:07.000Z", "title": "Spatially Resolving the Very High Energy emission from MGRO J2019+37 with VERITAS", "authors": [ "VERITAS Collaboration" ], "comment": "9 pages, 8 figures, accepted for publication in the Astrophysical Journal", "categories": [ "astro-ph.HE" ], "abstract": "We present very high energy (VHE) imaging of MGRO J2019+37 obtained with the VERITAS observatory. The bright extended ($\\sim2^{\\circ}$) unidentified Milagro source is located towards the rich star formation region Cygnus-X. MGRO J2019+37 is resolved into two VERITAS sources. The faint point-like source VER J2016+371 overlaps CTB 87, a filled-center remnant (SNR) with no evidence of a supernova remnant shell at the present time. Its spectrum is well fit in the $0.65 - 10$ TeV energy range by a power-law model with photon index $2.3\\pm0.4$. VER J2019+368 is a bright extended ($\\sim1^{\\circ}$) source, that likely accounts for the bulk of the Milagro emission and is notably coincident with PSR J2021+3651 and the star formation region Sh 2-104. Its spectrum in the range $1-30$ TeV is well fit with a power-law model of photon index $1.75\\pm0.3$, among the hardest values measured in the VHE band, comparable to that observed near Vela-X. We explore the unusual spectrum and morphology in the radio and X-ray bands to constrain possible emission mechanisms for this source.", "revisions": [ { "version": "v1", "updated": "2014-04-07T16:31:07.000Z" } ], "analyses": { "keywords": [ "high energy emission", "spatially resolving", "rich star formation region cygnus-x", "power-law model", "star formation region sh" ], "tags": [ "journal article" ], "publication": { "doi": "10.1088/0004-637X/788/1/78", "journal": "The Astrophysical Journal", "year": 2014, "month": "Jun", "volume": 788, "number": 1, "pages": 78 }, "note": { "typesetting": "TeX", "pages": 9, "language": "en", "license": "arXiv", "status": "editable", "inspire": 1288854, "adsabs": "2014ApJ...788...78A" } } }