G. Castelletti

TL;DR: In this paper, the authors investigated two multi-shell galactic supernova remnants (SNRs), Kes79 and G352.7-0.1, to understand the causes of such morphology.

TL;DR: In this article, the morphology at low radio frequencies of the supernova remnant IC443 and accurately established its radio continuum spectral properties were investigated in detail, and it was shown that thermal absorption at 74 MHz is responsible for the localized spectral index flattening observed along the eastern border of IC443.

TL;DR: In this article, Chandra observations of the region around the putative pulsar, CXOU J061705.3+222127, in the supernova remnant IC443 reveal an ~5$^{\prime\prime}$-radius ring-like structure surrounding the pulsar and a jet-like feature oriented roughly north-south across the ring and through pulsar's location at 06$^{rm h}$17$€{\rm m}$5.52$^

TL;DR: In this article, the first detailed full view of Puppis A in X-rays was obtained by combining the missing regions in the southern half of the supernova remnant (SNR) and combined with existing XMM-Newton and Chandra data.