Achromatic rapid flares in hard X-rays in the $\gamma$-ray binary LS I +61-303
Enzo A. Saavedra, Gustavo E. Romero, Valenti Bosch-Ramon, Elina Kefala

TL;DR
This study reports rapid achromatic hard X-ray flares in the gamma-ray binary LS I +61 303, suggesting synchrotron emission from relativistic electrons affected by dynamic changes in the shock region.
Contribution
First detection of rapid achromatic X-ray flares in LS I +61 303, linking variability to shock region dynamics and relativistic flow effects.
Findings
Detected two ks-scale achromatic flares in hard X-rays.
Flares likely caused by changes in the size or motion of the emitting region.
Synchrotron emission from relativistic electrons in a shocked pulsar wind.
Abstract
We report on the presence of very rapid hard X-ray variability in the -ray binary LS I +61 303. The results were obtained by analysing NuSTAR data, which show two achromatic strong flares on ks time-scales before apastron. The Swift-BAT orbital X-ray light curve is also presented, and the NuSTAR data are put in the context of the system orbit. The spectrum and estimated physical conditions of the emitting region indicate that the radiation is synchrotron emission from relativistic electrons, likely produced in a shocked pulsar wind. The achromaticity suggests that losses are dominated by escape or adiabatic cooling in a relativistic flow, and the overall behaviour in hard X-rays can be explained by abrupt changes in the size of the emitting region and/or its motion relative to the line of sight, with Doppler boosting potentially being a prominent effect. The rapid changes of the…
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