{ "id": "0907.5415", "version": "v1", "published": "2009-07-30T20:03:52.000Z", "updated": "2009-07-30T20:03:52.000Z", "title": "X-Ray Monitoring of Ultraluminous X-Ray Sources", "authors": [ "Philip Kaaret", "Hua Feng" ], "comment": "4 pages, to appear in ApJ", "categories": [ "astro-ph.HE" ], "abstract": "X-ray monitoring observations were performed with the Swift observatory of the ultraluminous X-ray sources Holmberg IX X-1, NGC 5408 X-1, and NGC 4395 X-2 and also of the nuclear X-ray source in NGC 4395. Holmberg IX X-1 remains in the hard X-ray spectral state as its flux varies by a factor of 7 up to an (isotropic) luminosity of 2.8E40 erg/s. This behavior may suggest an unusually massive compact object. We find excess power at periods near 60 days and 28 days in the X-ray emission from Holmberg IX X-1. Additional monitoring is required to test the significance of these signals. NGC 5408 X-1 and NGC 4395 X-2 appear to remain in the soft spectral state found by Chandra and XMM with little variation in spectral hardness even as the luminosity changes by a factor of 9. We found an outburst from the nuclear source in NGC 4395 reaching an X-ray luminosity of 9E40 erg/s, several times higher than any previously reported.", "revisions": [ { "version": "v1", "updated": "2009-07-30T20:03:52.000Z" } ], "analyses": { "keywords": [ "x-ray monitoring", "ultraluminous x-ray sources holmberg ix", "hard x-ray spectral state", "nuclear x-ray source", "soft spectral state" ], "tags": [ "journal article" ], "publication": { "doi": "10.1088/0004-637X/702/2/1679", "journal": "The Astrophysical Journal", "year": 2009, "month": "Sep", "volume": 702, "number": 2, "pages": 1679 }, "note": { "typesetting": "TeX", "pages": 4, "language": "en", "license": "arXiv", "status": "editable", "inspire": 827543, "adsabs": "2009ApJ...702.1679K" } } }