Article: Recent findings from E.G. Berezhko and co-authors highlight research in astrophysics.

"The properties of the Galactic supernova remnant (SNR) RX J0852.0-4622 are theoretically analysed. An explicitly time-dependent, nonlinear kinetic model of cosmic ray (CR) acceleration in SNRs is used to describe the properties of SNR RX J0852.0-4622, the accelerated CRs, and the nonthermal emission," scientists writing in the journal Astronomy & Astrophysics report.

"The source is assumed to be at a distance of approximate to 1 kpc in the wind bubble of a massive progenitor star. An estimate of the thermal X-ray flux in this configuration is given. We find that the overall synchrotron spectrum of RX J0852.0-4622 as well as the filamentary structures in hard ...

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