Synchrotron emission model of RX J1856.5-3754

A plasma emission model is presented interpreting the observational properties of RX J1856.5-3754. In particular, on the basis of the Vlasov’s kinetic equation we study the process of the quasi-linear diffusion (QLD) developed by means of the cyclotron instability. This mechanism provides simultaneous generation of optical and X-ray emission on the light cylinder scales, in one location of the pulsar magnetosphere. It is assumed that the observed X-ray spectrum of this source is generated via the synchrotron mechanism. A different approach of the synchrotron theory is considered, giving a spectral energy distribution that is in a good agreement with the observational data.

► We present emission model explaining observational properties of RX J1856.5-3754.
► The observed X-ray spectrum is explained by the synchrotron emission.
► The cyclotron instability causes appearance of synchrotron emission.
► The model spectrum fits well the measured one.