activity
20242026
collaborators

8 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

He-star donor pathway for the hypervelocity star D6-2

Abinaya Swaruba Rajamuthukumar, Ruediger Pakmor, Stephen Justham +2

Type Ia supernovae are thermonuclear explosions of white dwarfs, yet the nature of their progenitor systems remains uncertain. Recent discoveries of hypervelocity stars provide uni…

astro-ph.SR2025

The role of triple evolution in the formation of LISA double white dwarfs

Abinaya Swaruba Rajamuthukumar, Valeriya Korol, Jakob Stegmann +5

Galactic double white dwarfs will be prominent gravitational-wave sources for the Laser Interferometer Space Antenna (LISA). While previous studies have primarily focused on format…

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

Prompt stellar and binary black hole mergers in tight triples: Insights from chemically homogeneous evolution

Alejandro Vigna-Gómez, Evgeni Grishin, Jakob Stegmann +7

Short-period massive binary stars are predicted to undergo chemically homogeneous evolution (CHE), making them prime candidates for producing binary black holes (BBHs) that may mer…