TeV -ray observations of the young synchrotron-dominated SNRs G1.9+0.3 and G330.2+1.0 with H.E.S.S.
A. Abramowski, Felix Aharonian, F. Ait Benkhali, A. G. Akhperjanian et autres
The non-thermal nature of the X-ray emission from the shell-type supernova remnants (SNRs) G1.9+0.3 and G330.2+1.0 is an indication of intense particle acceleration in the shock fronts of both objects. This suggests that the SNRs are prime candidates for very-high-energy (VHE; E …
fr, gb, de, au, ie, am, pl, se, at, Afrique du Sud, Namibie (code pays fourni par la source)
23 citations
Monthly Notices of the Royal Astronomical Society