activity
20242026
collaborators

6 papers

astro-ph.HE2026

Violent mergers revisited: The origin of the fastest stars in the Galaxy

Rüdiger Pakmor, Ken J. Shen, Aakash Bhat +12

Binary systems of two carbon-oxygen white dwarfs are one of the most promising candidates for the progenitor systems of Type Ia supernovae. Violent mergers, where the primary white…

astro-ph.SR2025

Evolution of binaries containing a hot subdwarf and a white dwarf to double white dwarfs, and double detonation supernovae with hypervelocity runaway stars

Abinaya Swaruba Rajamuthukumar, Evan B. Bauer, Stephen Justham +3

Compact binaries containing hot subdwarfs and white dwarfs have the potential to evolve into a variety of explosive transients. These systems could also explain hypervelocity runaw…

astro-ph.SR2025

Violent mergers can explain the inflated state of some of the fastest stars in the Galaxy

Aakash Bhat, Rüdiger Pakmor, Ken J. Shen +2

A significant number of hypervelocity stars with velocities between km/s have recently been observed. The only plausible explanation so far is that they have been produ…

astro-ph.SR2025

Spectroscopic and kinematic analyses of a warm survivor of a D6 supernova

Mark A. Hollands, Ken. J. Shen, Roberto Raddi +3

SDSSJ163712.21+363155.9 is a candidate hyper-runaway star, first identified from its unusual spectrum in the Sloan Digital Sky Survey, which exhibits oxygen, magnesium, and silicon…

astro-ph.SR2025

The dearth of high-mass hydrogen-atmosphere metal-polluted white dwarfs within 40 pc

Tim Cunningham, Pier-Emmanuel Tremblay, Mairi O'Brien +7

We present a population synthesis model which addresses the different mass distributions of the metal-polluted and non-metal-polluted hydrogen-atmosphere white dwarfs identified in…

astro-ph.SR2024

A gravitational wave detectable candidate Type Ia supernova progenitor

Emma T. Chickles, Kevin B. Burdge, Joheen Chakraborty +37

Type Ia supernovae, critical for studying cosmic expansion, arise from thermonuclear explosions of white dwarfs, but their precise progenitor pathways remain unclear. Growing evide…