{ "id": "1105.4761", "version": "v1", "published": "2011-05-24T13:37:11.000Z", "updated": "2011-05-24T13:37:11.000Z", "title": "The non-thermal, time-variable radio emission from Cyg OB2 # 5: A wind-collision region", "authors": [ "Gisela Ortiz-Leon", "Laurent Loinard", "Luis F. Rodriguez", "Amy J. Mioduszewski", "Sergio A. Dzib" ], "comment": "Accepted for publication in The Astrophysical Journal", "categories": [ "astro-ph.GA", "astro-ph.SR" ], "abstract": "The radio emission from the well-studied massive stellar system Cyg OB2 #5 is known to fluctuate with a period of 6.7 years between a low-flux state when the emission is entirely of free-free origin, and a high-flux state when an additional non-thermal component (of hitherto unknown nature) appears. In this paper, we demonstrate that the radio flux of that non-thermal component is steady on timescales of hours, and that its morphology is arc-like. This shows that the non-thermal emission results from the collision between the strong wind driven by the known contact binary in the system, and that of an unseen companion on a somewhat eccentric orbit with a 6.7-yr period and a 5 to 10 mas semi-major axis. Together with the previously reported wind-collision region located about 0.8 arcsec to the north-east of the contact binary, Cyg OB2 #5 appears to be the only multiple system known so far to harbor two radio-imaged wind-collision regions.", "revisions": [ { "version": "v1", "updated": "2011-05-24T13:37:11.000Z" } ], "analyses": { "keywords": [ "wind-collision region", "time-variable radio emission", "massive stellar system cyg ob2", "non-thermal component", "contact binary" ], "tags": [ "journal article" ], "publication": { "doi": "10.1088/0004-637X/737/1/30", "journal": "The Astrophysical Journal", "year": 2011, "month": "Aug", "volume": 737, "number": 1, "pages": 30 }, "note": { "typesetting": "TeX", "pages": 0, "language": "en", "license": "arXiv", "status": "editable", "inspire": 901128, "adsabs": "2011ApJ...737...30O" } } }