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• W3125341018 abstract "The prototypical post-core-collapse globular cluster M15 provides an ideal environment for the formation of exotic binaries, it being already known to contain a luminous LMXB (X2127+119, optically identified with the 17.1-h eclipsing binary AC211) and 6 millisecond-pulsars in the core. However, the X-ray properties of X2127+119 are strange in that it appears to be a high inclination accretion disc corona source (ADC) from which we only see scattered X-radiation, and yet it has produced extremely luminous type I X-ray bursts, which may or may not have come from AC211. We have therefore examined the ∼5-year RXTE/ASM light curve of this object in order to search for long-term modulations which might shed light on this unusual behaviour, and which led to our discovery of further X-ray bursts. Furthermore, we have used archival HST UV images of the M15 core to search for other variable objects which might indicate the presence of a second LMXB. From these we have found one highly variable (>5 mag) object which we interpret as a dwarf nova." @default.
• W3125341018 created "2021-02-01" @default.
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• W3125341018 date "2002-01-01" @default.
• W3125341018 modified "2023-09-27" @default.
• W3125341018 title "X-ray and UV variability in the core of : the nature of /" @default.
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• W3125341018 doi "https://doi.org/10.1016/s1384-1076(01)00087-2" @default.
• W3125341018 hasPublicationYear "2002" @default.
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