Abstract Rayleigh–Taylor (RT) and Richtmyer–Meshkov (RM) instabilities are well-known
pathways towards turbulent mixing layers, in many cases characterized by significant mass …

▪ Abstract The temporal evolution of the optical spectra of various types of supernovae (SNe)
is illustrated, in part to aid observers classifying supernova candidates. Type II SNe are …

Abstract Type Ia supernovae (SNe Ia) play a key role in the fields of astrophysics and
cosmology. It is widely accepted that SNe Ia arise from thermonuclear explosions of white …

We conduct an analytic and numerical study of the dynamics of supernova remnant (SNR)
evolution from the ejecta-dominated stage through the Sedov-Taylor (ST) stage, the stages …

JCW had long wanted to write a new monograph on supernovae. Despite an immense
explosion in the literature and many review articles, there had not been one since that of …

We present the results of numerical studies of supernova remnant evolution and its effects
on galactic and globular cluster evolution. We show that parameters such as the density and …

The conditions for validity and the limitations of experiments intended to simulate
astrophysical hydrodynamics are discussed, with application to some ongoing experiments …

We present three-dimensional hydrodynamic simulations of the evolution of core-collapse
supernovae (SN) from blast-wave initiation by the neutrino-driven mechanism to shock …

We describe a numerical code to solve the equations for ideal magnetohydrodynamics
(MHD). It is based on an explicit finite difference scheme on an Eulerian grid, called the Total …

Context. The Orion Molecular Cloud is the nearest massive-star forming region. Massive
stars have profound effects on their environment due to their strong radiation fields and …