The observable characteristics and subsequent evolution of young stellar populations is
dominated by their massive stars. As our understanding of those massive stars and the …

Neutrinos are known to play important roles in many astrophysical scenarios from the early
period of the big bang to current stellar evolution being a unique messenger of the fusion …

Most massive stars are members of a binary or a higher-order stellar system, where the
presence of a binary companion can decisively alter their evolution via binary interactions …

We present results from a self-consistent, non-rotating core-collapse supernova simulation
in three spatial dimensions using a binary evolution progenitor model of SN 1987A. This …

Our understanding of the convective-engine paradigm driving core-collapse supernovae
has been used for two decades to predict the remnant mass distribution from stellar …

With the remarkable success of the Ligo-Virgo-Kagra consortium in detecting binary black
hole mergers, it has become possible to use the population properties to constrain our …

In binary black hole mergers from isolated binary-star evolution, both black holes are from
progenitor stars that have lost their hydrogen-rich envelopes by binary mass transfer …

Understanding the astrophysical phenomena involving compact objects requires an insight
about the engine behind the core-collapse supernovae (SNe) and the fate of the stellar …

Common envelope (CE) evolution is an outstanding open problem in stellar evolution,
critical to the formation of compact binaries including gravitational-wave sources. In the" …

Most massive stars are born in binaries close enough for mass transfer episodes. These
modify the appearance, structure, and future evolution of both stars. We compute the …