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 …

This paper presents a short review on the current state of SN Ia progenitor origin. Type Ia
supernova explosions (meaning thermonuclear disruption of a white dwarf) are observed to …

We investigate whether pure deflagration models of Chandrasekhar-mass carbon–oxygen
white dwarf stars can account for one or more subclass of the observed population of Type …

Type Iax supernovae are stellar explosions that are spectroscopically similar to some type Ia
supernovae at the time of maximum light emission, except with lower ejecta velocities,. They …

We present the implementation of updated stellar evolution recipes in the codes nbody6++
gpu, mocca, and mcluster. We test them through numerical simulations of star clusters …

Context. Manganese is predominantly synthesised in Type Ia supernova (SN Ia) explosions.
Owing to the entropy dependence of the Mn yield in explosive thermonuclear burning, SNe …

The ejected mass distribution of Type Ia supernovae (SNe Ia) directly probes progenitor
evolutionary history and explosion mechanisms, with implications for their use as …

Stellar evolution models predict the existence of hybrid white dwarfs (WDs) with a carbon–
oxygen core surrounded by an oxygen–neon mantle. Being born with masses∼ 1.1 M⊙ …

We conduct the first 3D hydrodynamic simulations of oxygen–neon white dwarf–neutron
star/black hole mergers (ONe WD–NS/BH mergers). Such mergers constitute a significant …

Recent surveys show that wide (> 104 AU) binaries and triples are abundant in the field. We
study the long-term evolution of wide hierarchical triple systems and the role played by the …