Synchrotron emission model of RX J1856.5-3754

Details Synchrotron emission model of RX J1856.5-3754 Synchrotron emission model of RX J1856.5-3754

Feb 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012newa...17..227c&link_type=abstract

New Astronomy, Volume 17, Issue 2, p. 227-231.

Astronomy and Astrophysics

Astronomy

Scientific paper

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.

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