Most supernova explosions accompany the death of a massive star. These explosions give
birth to neutron stars and black holes, and eject solar masses of heavy elements. However …

We have conducted 19 state-of-the-art 3D core-collapse supernova simulations spanning a
broad range of progenitor masses. This is the largest collection of sophisticated 3D …

Supernova (SN) explosions have been sought for decades as a possible source of dust in
the Universe, providing the seeds of galaxies, stars, and planetary systems. SN 1987A offers …

In the transitional mass range (~ 8–10 solar masses) between white dwarf formation and
iron core-collapse supernovae, stars are expected to produce an electron-capture …

We explore the three-dimensional properties of convective, luminous (L≈ 10 4.5–10 5 L⊙),
hydrogen-rich envelopes of red supergiants (RSGs) based on radiation hydrodynamic …

Linking supernovae to their progenitors is a powerful method for furthering our
understanding of the physical origin of their observed differences while at the same time …

The present study is the first of a series of three papers where we characterise the type II
supernovae (SNe II) from the Carnegie Supernova Project-I to understand their diversity in …

Abstract Using Modules for Experiments in Stellar Astrophysics (MESA)+ STELLA, we show
that very different physical models can adequately reproduce a specific observed Type II …

The majority of massive stars, which are the progenitors of core-collapse supernovae (SNe),
are found in close binary systems. In a previous work, we modeled the fraction of hydrogen …

The minimum initial mass required for a star to explode as an Fe core collapse supernova,
typically denoted M mas, is an important quantity in stellar evolution because it defines the …