We report the discovery of J0624–6948, a low-surface brightness radio ring, lying between
the Galactic Plane and the large magellanic cloud (LMC). It was first detected at 888 MHz …

Abstract Type Ia supernovae (SNe) are believed to be caused by the thermonuclear
explosion of a white dwarf (WD), but the nature of the progenitor system (s) is still unclear …

The recent advanced LIGO/Virgo detections of gravitational waves (GWs) from stellar binary
black hole (BBH) mergers, in particular GW190521, which is potentially associated with a …

By using surface brightness maps of Tycho's supernova remnant (SNR) in radio and X-rays,
along with the properties of thermal and synchrotron emission, we have derived the …

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 …

The contribution of galactic supernova remnants (SNRs) to the origin of cosmic rays (CRs) is
an important open question in modern astrophysics. Broadband nonthermal emission is a …

Context. Jets of active galactic nuclei are potential accelerators of ultra high-energy cosmic
rays. Supernovae can occur inside these jets and contribute to cosmic ray acceleration …

Young massive stars in compact stellar clusters could end their evolution as core-collapse
supernovae a few million years after the cluster was built. The blast wave of a supernova …

Ultra-short laser pulses (1030 nm/230 fs) were used to laser ablate the surface of crystalline
sapphire (Al2O3) at high intensity per pulse 20–200 TW/cm 2/pulse. Laser-ablated patterns …

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 …