The detected polarized radio emission from the remnant of SN1987A opens the possibility to
unveil the structure of the pre-supernova (pre-SN) magnetic field (MF) in the circumstellar …

Supernova remnants (SNRs) can be rich sources of information on the parent SN
(supernova) explosion. Thus, investigating the transition from the phase of SN to that of SNR …

We consider the influence of a fluctuating magnetic field on to the structure formation and
instabilities of radiatively cooling blast waves. The study is based on an example of optically …

The large, faint supernova remnant (SNR) G70. 0–21.5 is believed to be the result of a Type
Ia supernova some 90,000 yr ago at a distance of∼ 1 kpc based on the Gaia proper motion …

The influence of neutrals on the development of multidimensional dense-shell instabilities in
supernova remnants is investigated. We present a model in which the neutrals are …

Near the ends of their lives, supernova remnants (SNRs) enter a" radiative phase," when
efficient cooling of the postshock gas slows expansion. Understanding SNR evolution at this …

The evolution of shocks induced by massive stars does not depend only on the ambient
magnetic field strength, but also on its orientation. In the present work, the dynamics of a …

The self-similar dynamics of the collision between radiative and adiabatic supersonic planar
flows are performed assuming homogeneous radiation cooling. New self-similar solutions …

The ionization effect on both the evolution and internal structure of a blast wave (BW) is
determined in laboratory conditions. In a first step, the Rankine–Hugoniot equations …

We study the polarized radio emission from young Type Ia supernova remnants by means of
three-dimensional numerical MHD simulations and the assumption of relativistic electron …