Multidimensional simulations show that non-radial, turbulent, fluid motion is a fundamental
component of the core-collapse supernova explosion mechanism. Neutrino-driven …

Context. The remnants of core-collapse supernovae (SNe) are probes of the physical
processes associated with their parent SNe. Aims. Here we aim to explore to which extent …

Large-scale Mixing in a Violent Oxygen–Neon Shell Merger Prior to a Core-collapse
Supernova - IOPscience This site uses cookies. By continuing to use this site you agree to …

ABSTRACT A critical relation in the study of neutron star cooling is the one between surface
temperature and interior temperature. This relation is determined by the composition of the …

The properties (temperature, density, chemical composition, velocity) of hot astrophysical
plasma and the physical processes affecting them (heating/cooling, turbulence, shocks …

Neutrino interactions with stellar material are widely believed to be fundamental to the
explosion of massive stars. However, this important process has remained difficult to confirm …

We present a new optical sample of three Supernova Remnants (SNRs) and 16 Supernova
Remnant (SNR) candidates in the Large Magellanic Cloud (LMC). These objects were …

We present a hyperspectral cube of the Crab Nebula obtained with the imaging Fourier
transform spectrometer SITELLE on the Canada–France–Hawaii telescope. We describe …

We present a three-dimensional kinematic reconstruction of the optically emitting, oxygen-
rich ejecta of supernova remnant N132D in the Large Magellanic Cloud (LMC). Data were …

We have carried out Very Large Array imaging and a Fermi timing analysis of the 115 ms γ-
ray and radio pulsar PSR J0002+ 6216. We found that the pulsar lies at the apex of a …