Type Ia supernovae (SNe Ia) are important distance indicators, element factories, cosmic-ray
accelerators, kinetic-energy sources in galaxy evolution, and end points of stellar binary …

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 …

Monitoring of vibrational eigenmodes of an elastic body excited by gravitational waves was
one of the first concepts proposed for the detection of gravitational waves. At laboratory …

Type Ia supernovae have been used empirically as 'standard candles' to demonstrate the
acceleration of the expansion of the Universe,, even though fundamental details, such as the …

One of the most important questions regarding the progenitor systems of Type Ia
supernovae (SNe Ia) is whether mergers of two white dwarfs can lead to explosions that …

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 …

Context. The study of Type Ia supernovae (SNIa) has lead to greatly improved insights into
many fields in astrophysics, eg cosmology, and also into the metal enrichment of the …

Type Ia supernovae are thought to result from a thermonuclear explosion of an accreting
white dwarf in a binary system,, but little is known of the precise nature of the companion star …

Abstract Using the Zwicky Transient Facility alert stream, we are conducting a large
spectroscopic campaign to construct a complete, volume-limited sample of transients …

Type Ia supernovae arise from the thermonuclear explosion of white-dwarf stars that have
cores of carbon and oxygen,. The uniformity of their light curves makes these supernovae …