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- W2068234414 abstract "We report our analysis of X-ray data on M101 ULX-1, concentrating on high-state Chandra and XMM-Newton observations. We find that the high state of M101 ULX-1 may have a preferred recurrence timescale. If so, the underlying clock may have periods around 160 or 190 days, or possibly around 45 days. Its short-term variations resemble those of X-ray binaries at high accretion rates. If this analogy is correct, we infer that the accretor is a 20-40 M☉ object. This is consistent with our spectral analysis of the high-state spectra of M101 ULX-1, from which we find no evidence for an extreme (>1040 ergs s-1) luminosity. We present our interpretation in the framework of a high-mass X-ray binary system consisting of a B supergiant mass donor and a large stellar-mass black hole." @default.
- W2068234414 created "2016-06-24" @default.
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- W2068234414 date "2005-12-01" @default.
- W2068234414 modified "2023-09-25" @default.
- W2068234414 title "The X‐Ray Properties of M101 ULX‐1 = CXOKM101 J140332.74+542102" @default.
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- W2068234414 doi "https://doi.org/10.1086/497110" @default.
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