{ "id": "2411.07459", "version": "v1", "published": "2024-11-12T00:51:49.000Z", "updated": "2024-11-12T00:51:49.000Z", "title": "The long-term variability of a population of ULXs monitored by Chandra", "authors": [ "Hannah P. Earnshaw", "Gauri Patti", "Murray Brightman", "Rajath Sathyaprakash", "Dominic J. Walton", "Felix Fuerst", "Timothy P. Roberts", "Fiona A. Harrison" ], "comment": "7 pages, 4 figures, to be published in Proceedings of the XMM-Newton Workshop 2024 \"The X-ray Mysteries of Neutron Stars and White Dwarfs\", Astronomische Nachrichten, in press", "categories": [ "astro-ph.HE" ], "abstract": "We present preliminary results of a Chandra Large Program to monitor the ultraluminous X-ray source (ULX) populations of three nearby, ULX-rich galaxies over the course of a year, finding the ULX population to show a variety of long-term variability behaviours. Of a sample of 36 ULXs, some show persistent or moderately variable flux, often with a significant relationship between hardness and luminosity, consistent with a supercritically accreting source with varying accretion rates. Six show very high-amplitude variability with no strong relationship between luminosity and hardness, though not all of them show evidence of any long-term periodicity, nor of the bimodal distribution indicative of the propeller effect. We find evidence of additional eclipses for two previously-identified eclipsing ULXs. Additionally, many sources that were previously identified as ULXs in previous studies were not detected at ULX luminosities during our monitoring campaign, indicating a large number of transient ULXs.", "revisions": [ { "version": "v1", "updated": "2024-11-12T00:51:49.000Z" } ], "analyses": { "keywords": [ "population", "chandra large program", "long-term variability behaviours", "luminosity", "additional eclipses" ], "note": { "typesetting": "TeX", "pages": 7, "language": "en", "license": "arXiv", "status": "editable" } } }