collaborators

6 papers

astro-ph.HE2026

Hyperaccreting Magnetised Neutron Stars inside Rotating Massive Envelopes: Low-Power Jets and Precursor Flares

Patrick Chi-Kit Cheong, Christopher L. Fryer, David Radice

The engulfment of a neutron star (NS) by a massive companion initiates a highly dynamic common-envelope (CE) evolution phase. As the NS spirals into the dense stellar core, it is s…

astro-ph.HE2026

Hyperaccreting Neutron Stars inside Massive Envelopes: The Implausibility of Thorne-Żytkow Objects

Patrick Chi-Kit Cheong, David Radice, Christopher L. Fryer

The evolution of neutron stars (NSs) embedded within massive stellar envelopes is a critical phase in binary stellar evolution, potentially leading to the formation of Thorne-Å»ytk…

astro-ph.HE2026

Production of heavy -elements and Ti in Cas A: comparison to abundances from 1D core-collapse supernova models and evidence for Carbon-Oxygen shell mergers

Luca Boccioli, Lorenzo Roberti, Chris L Fryer +3

The merger between the carbon (C) and oxygen (O) shells hours to days before the collapse of a massive star significantly changes its nucleosynthesis, which is reflected in the ele…

astro-ph.HE2026

Angular momentum drives proton-rich nucleosynthesis in hyperaccreting neutron stars in common envelopes

Alexander D. Hall-Smith, Sophie E. D. Abrahams, Alison M. Laird +3

Interacting binaries can produce a wide range of exotic systems, including X-ray binaries and merging neutron stars, through a mass transfer phase called Common Envelope (CE) evolu…

astro-ph.HE2025

Revisiting the Supernova Engines in the 3C 397 and W49B Supernova Remnants

Cole Treyturik, Chelsea Braun, Samar Safi-Harb +2

The nature of the supernova remnants (SNRs) 3C 397 and W49B has long been a subject of debate, with prior studies offering conflicting interpretations between thermonuclear and cor…

astro-ph.SR2025

Production of radioactive Na in core-collapse supernovae: the Ne-E(L) component in presolar grains and its possible consequences on supernova observations

M. Pignatari, S. Amari, P. Hoppe +8

Presolar graphite grains carry the isotopic signatures of their parent stars. A significant fraction of presolar graphites shows isotopic abundance anomalies relative to solar for…