@article {22722,
	title = {A two-zone model for the emission from <ASTROBJ>RX J1713.7-3946</ASTROBJ>},
	volume = {462},
	year = {2007},
	month = {2007/01/1},
	pages = {173 - 177},
	abstract = {Aims:We study the acceleration and radiation of charged particles in the shock waves of supernova remnants using a recent version of the "box model". According to this, particles are accelerated in an energy-dependent region around the shock by the first order Fermi mechanism and lose energy through radiation. <BR />Methods: The particle distribution function is obtained from a spatially averaged kinetic equation that treats the energy losses self-consistently. There exists also a second population that consists of those particles that escape behind the shock where they also radiate. The energy distribution of this population is calculated in a similar manner. <BR />Results: The application of the model to the supernova remnant <ASTROBJ>RX J1713.7-3946</ASTROBJ>, which was recently confirmed as a TeV source by HESS, shows that the X-ray emission can be attributed to electron synchrotron radiation while in γ-rays there are contributions from both electrons and protons, with protons playing the dominant role. Additionally, there are strong indications that particles diffuse in turbulence that has a Kolmogorov spectrum.},
	keywords = {acceleration of particles, Astrophysics, cosmic rays, ISM: supernova remnants, radiation mechanisms: non-thermal},
	isbn = {0004-6361},
	url = {https://ui.adsabs.harvard.edu/abs/2007A\&A...462..173M},
	author = {Moraitis, K. and Mastichiadis, A.}
}
