{ "id": "1409.6664", "version": "v1", "published": "2014-09-23T16:47:00.000Z", "updated": "2014-09-23T16:47:00.000Z", "title": "A $\\sim$100 mHz QPO in the X-ray emission from IGR J17361-4441", "authors": [ "E. Bozzo", "A. Papitto", "C. Ferrigno", "T. M. Belloni" ], "comment": "Submitted to A&A on 2014 August 10. Revised according to referee's suggestions", "categories": [ "astro-ph.HE" ], "abstract": "IGR J17361-4441 was discovered by INTEGRAL undergoing its first detectable X-ray outburst in 2011 and initially classified as an accreting X-ray binary in the globular cluster NGC 6388. A reanalysis of the outburst data collected with INTEGRAL and Swift suggested that the enhanced X-ray emission from IGR J17361-4441 could have been due to a rare tidal disruption event of a terrestrial- icy planet by a white dwarf. In this letter we report on the analysis of XMM-Newton data collected in 2011 during the outburst from IGR J17361-4441. Our analysis revealed the presence of a $\\sim$100 mHz quasi-periodic oscillation in the X-ray emission from the source and confirmed the presence of a soft thermal component (kT$\\sim$0.08 keV) in its spectrum. We discuss these findings in the context of the different possibilities proposed to explain the nature of IGR J17361-4441.", "revisions": [ { "version": "v1", "updated": "2014-09-23T16:47:00.000Z" } ], "analyses": { "keywords": [ "x-ray emission", "mhz qpo", "rare tidal disruption event", "first detectable x-ray outburst", "mhz quasi-periodic oscillation" ], "tags": [ "journal article" ], "publication": { "doi": "10.1051/0004-6361/201424788", "journal": "Astronomy and Astrophysics", "year": 2014, "month": "Oct", "volume": 570 }, "note": { "typesetting": "TeX", "pages": 0, "language": "en", "license": "arXiv", "status": "editable", "inspire": 1318638, "adsabs": "2014A&A...570L...2B" } } }