{ "id": "1409.1985", "version": "v1", "published": "2014-09-06T06:19:59.000Z", "updated": "2014-09-06T06:19:59.000Z", "title": "The orbital period of Swift J1816.7-1613 revealed by the Swift-BAT telescope", "authors": [ "V. La Parola", "A. Segreto", "G. Cusumano", "N. Masetti", "A. D'Ai", "A. Melandri" ], "comment": "6 pages, 6 figures. Accepted for publication on MNRAS", "categories": [ "astro-ph.HE" ], "abstract": "We have analyzed the Swift data relevant to the high mass X-ray binary Swift J1816.7-1613. The timing analysis of the BAT survey data unveiled a modulation at a period of P_0=118.5+/-0.8 days that we interpret as the orbital period of the X-ray binary system. The modulation is due to a sequence of bright flares, lasting ~30 d, separated by long quiescence intervals. This behavior is suggestive of a Be binary system, where periodic or quasi-periodic outbursts are the consequence of an enhancement of the accretion flow from the companion star at the periastron passage. The position of Swift J1816.7-1613 on the Corbet diagram strengthens this hypothesis. The broad band 0.2-150 keV spectrum is well modeled with a strongly absorbed power-law with a flat photon index Gamma~ 0.2 and a cut-off at ~ 10 keV.", "revisions": [ { "version": "v1", "updated": "2014-09-06T06:19:59.000Z" } ], "analyses": { "keywords": [ "orbital period", "swift-bat telescope", "high mass x-ray binary swift", "mass x-ray binary swift j1816", "binary system" ], "tags": [ "journal article" ], "publication": { "doi": "10.1093/mnrasl/slu147", "journal": "Monthly Notices of the Royal Astronomical Society", "year": 2014, "month": "Nov", "volume": 445, "number": 1 }, "note": { "typesetting": "TeX", "pages": 6, "language": "en", "license": "arXiv", "status": "editable", "inspire": 1315395, "adsabs": "2014MNRAS.445L.119L" } } }