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- W1918302017 abstract "A few Galactic Low Mass X-Ray Binaries (LMXBs) have shown drastically evolving X-ray and/or optical orbital light curves. In two short-period LMXBs, MS 1603+2600 (= UW CrB, P orb = 111 min) and 4U 1916-053 (see e.g. Homer et al. 2001), the variations in the light curve morphology seem to be repeating in a periodic manner. We present first results of a photometric monitoring campaign of MS 1603+2600, showing evidence of a 5-day superorbital period in this yet unclassified source. The observations also unraveled optical flares, reminiscent of type I bursts, suggesting a neutron star primary." @default.
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- W1918302017 date "2004-01-01" @default.
- W1918302017 modified "2023-09-26" @default.
- W1918302017 title "Rapidly Evolving Light Curves of Low Mass X-Ray Binaries" @default.
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- W1918302017 doi "https://doi.org/10.1017/s0252921100152571" @default.
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