Fan, Z.H., Liu, S., Yuan, Q. and Fletcher, L. (2010) Lepton models for TeV emission from SNR RX J1713.7-3946. Astronomy and Astrophysics, 517(L4), (doi: 10.1051/0004-6361/201015169)
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Publisher's URL: http://dx.doi.org/10.1051/0004-6361/201015169
Abstract
<p><b>Aims:</b> SNR RX J1713.7-3946 is perhaps one of the best observed shell-type supernova remnants with emissions dominated by energetic particles accelerated near the shock front. The nature of the TeV emission, however, is an issue still open to investigation.</p> <p><b>Methods:</b> We carried out a systematic study of four lepton models for the TeV emission with the Markov chain Monte Carlo method.</p> <p><b>Results:</b> It is shown that current data already give good constraints on the model parameters. Two commonly used parametric models do not appear to fit the observed radio, X-ray, and γ-ray spectra. Models motivated by diffusive shock acceleration and by stochastic acceleration by compressive waves in the shock downstream give comparably good fits. The former has a sharper spectral cutoff in the hard X-ray band than the latter. Future observations with the HXMT and NuSTAR may distinguish these two models.</p>
Item Type: | Articles |
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Status: | Published |
Refereed: | Yes |
Glasgow Author(s) Enlighten ID: | Fletcher, Professor Lyndsay and Liu, Dr Siming |
Authors: | Fan, Z.H., Liu, S., Yuan, Q., and Fletcher, L. |
College/School: | College of Science and Engineering > School of Physics and Astronomy |
Journal Name: | Astronomy and Astrophysics |
Publisher: | EDP Sciences |
ISSN: | 0004-6361 |
ISSN (Online): | 1432-0746 |
Copyright Holders: | Copyright © 2010 EDP Sciences |
First Published: | First published in Astronomy and Astrophysics 517(L4) |
Publisher Policy: | Reproduced in accordance with the copyright policy of the publisher |
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