Journal Article

On the nature of the TeV emission from the supernova remnant SN 1006

Miguel Araya and Francisco Frutos

in Monthly Notices of the Royal Astronomical Society

Published on behalf of The Royal Astronomical Society

Volume 425, issue 4, pages 2810-2816
Published in print October 2012 | ISSN: 0035-8711
Published online October 2012 | e-ISSN: 1365-2966 | DOI: http://dx.doi.org/10.1111/j.1365-2966.2012.21580.x
On the nature of the TeV emission from the supernova remnant SN 1006

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We present a model for the non-thermal emission from the historical supernova remnant SN 1006. We constrain the synchrotron parameters of the model with archival radio and hard X-ray data. Our stationary emission model includes two populations of electrons, which is justified by multifrequency images of the object. From the set of parameters that predict the correct synchrotron flux we select those which are able to account, either partly or entirely, for the gamma-ray emission of the source as seen by HESS. We use the results from this model as well as the latest constraints imposed by the Fermi observatory and conclude that the TeV emission cannot be accounted for by π0 decay from high-energy ions with a single power-law distribution, of the form , and s ≳ 2.

Keywords: acceleration of particles; radiation mechanisms: non-thermal; ISM: individual objects: SN 1006; ISM: supernova remnants

Journal Article.  5508 words.  Illustrated.

Subjects: Astronomy and Astrophysics

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