Temporal features of LS I +61303 in hard X-rays from the Swift/BAT survey data
arXiv:1601.03260 · doi:10.1093/mnras/stv2716
Abstract
We study the long-term spectral and timing behaviour of LS I +61303 in hard X-rays (15--150 keV) using 10 years of survey data from the Burst Alert Telescope (BAT) monitor. We focus on the detection of long periodicities known to be present in this source in multiple wavelengths. We clearly detect three periods: the shorter one at 26.48 days is compatible with the orbital period of the system; the second, longer, periodicity at 26.93 days, is detected for the first time in X-rays and its value is consistent with an analogous temporal feature recently detected in the radio and in the gamma-ray waveband, and we associate it with a modulation caused by a precessing jet in this system. Finally, we find also evidence of the long-term periodicity at 1667 d, that results compatible with a beat frequency of the two close, and shorter, periodicities. We discuss our results in the context of the multi-band behaviour of the physical processes of this source.
5 pages, 8 figures. Published in MNRAS
References in corpus (6)
- VLBA images of the precessing jet of LSI+61303
- Long-term periodicity in LSI+61303 as beat frequency between orbital and precessional rate
- Intrinsic physical properties and Doppler boosting effects in LSI+61303
- Spectral analysis in orbital/superorbital phase space and hints of superorbital variability in the hard X-rays of LS I +61 303
- Discovery of a periodical apoastron GeV peak in LS I +61°303
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- A precessing stellar disk model for superorbital modulations of the gamma-ray binary LS I+61 303
- Achromatic rapid flares in hard X-rays in the -ray binary LS I +61-303
- Rapid X-ray variability of the gamma-ray binary LS I+61 303