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- W2102201368 abstract "We perform time-resolved spectroscopy of all the type I bursts from the Rapid Burster (MXB 1730-335) detected with the Rossi X-ray Timing Explorer. Type I bursts are detected at high accretion rates, up to sim 45% of the Eddington luminosity. We find evidence that bursts lacking the canonical cooling in their time-resolved spectra are, none the less, thermonuclear in nature. The type I bursting rate keeps increasing with the persistent luminosity, well above the threshold at which it is known to abruptly drop in other bursting low-mass X-ray binaries. The only other known source in which the bursting rate keeps increasing over such a large range of mass accretion rates is the 11 Hz pulsar IGR J17480$-$2446. This may indicate a similarly slow spin for the neutron star in the Rapid Burster." @default.
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- W2102201368 date "2013-03-12" @default.
- W2102201368 modified "2023-09-26" @default.
- W2102201368 title "Indications for a slow rotator in the Rapid Burster from its thermonuclear bursting behaviour" @default.
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- W2102201368 doi "https://doi.org/10.1093/mnras/stt312" @default.
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