Abstract
Abstract X-ray variabilities with spectral state transitions in bright low-mass X-ray binaries containing a neutron star are investigated by using the one-day bin light curves of MAXI/GSC (Gas Slit Camera) and Swift/BAT (Burst Alert Telescope). Four sources (4U 1636−536, 4U 1705−44, 4U 1608−52, and GS 1826−238) exhibited small-amplitude X-ray variabilities with spectral state transitions. Such “mini-outbursts” were characterized by smaller amplitudes (several times) and shorter duration (less than several tens of days) than those of “normal outbursts.” A theoretical model of disk instability by Mineshige and Osaki (PASJ, 37, 1, 1985) predicts both large-amplitude outbursts and small-amplitude variabilities. We interpret the normal outbursts as the former prediction of this model, and the mini-outbursts as the latter. Here, we can also call the mini-outburst a “purr-type outburst” referring to the theoretical work. We suggest that similar variabilities lasting for several tens of days without spectral state transitions, which are often observed in the hard state, may be repeats of mini-outbursts.
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