2007A&A...462..173M


Query : 2007A&A...462..173M

2007A&A...462..173M - Astronomy and Astrophysics, volume 462, 173-177 (2007/1-4)

A two-zone model for the emission from RX J1713.7-3946.

MORAITIS K. and MASTICHIADIS A.

Abstract (from CDS):

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. 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. The application of the model to the supernova remnant RX J1713.7-3946, 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.

Abstract Copyright:

Journal keyword(s): acceleration of particles - cosmic rays - radiation mechanisms: non-thermal - ISM: supernova remnants

Simbad objects: 2

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Number of rows : 2
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2024
#notes
1 SNR G347.3-00.5 SNR 17 12 27 -39 41.2     12.27     ~ 717 1
2 SNR G348.5+00.1 SNR 17 14 31.780 -38 28 34.50           ~ 219 3

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