activity
19972023
most citedThe Supernova -- Gamma-Ray Burst Connection

1.8k citations · 5.8k across the 40 of their papers we have counts for

collaborators
Showing 2021Show all

6 papers · 1 filter

astro-ph.SR20211 cited

Observational signatures of the surviving donor star in the double detonation model of Type Ia supernovae

Zheng-Wei Liu, Friedrich K. Roepke, Yaotian Zeng +1

The sub-Chandrasekhar mass double-detonation (DDet) scenario is a contemporary model for SNe Ia. The donor star in the DDet scenario is expected to survive the explosion and to be…

nucl-ex202122 cited

Advancement of Photospheric Radius Expansion and Clocked Type-I X-Ray Burst Models with the New MgAl Reaction Rate Determined at Gamow Energy

J. Hu, H. Yamaguchi, Y. H. Lam +34

We report the first (in)elastic scattering measurement of with the capability to select and measure in a broad energy range the proton resonances in Si…

astro-ph.HE202111 cited

X-ray burst ignition location on the surface of accreting X-ray pulsars: Can bursts preferentially ignite at the hotspot?

A. J. Goodwin, A. Heger, F. R. N. Chambers +2

Hotspots on the surface of accreting neutron stars have been directly observed via pulsations in the lightcurves of X-ray pulsars. They are thought to occur due to magnetic channel…

astro-ph.SR2021

The Pair-Instability Mass Gap for Black Holes

S. E. Woosley, Alexander Heger

Stellar evolution theory predicts a "gap" in the black hole birth function caused by the pair instability. Presupernova stars that have a core mass below some limiting value, Mlo,…

astro-ph.HE202155 cited

The final core collapse of pulsational pair instability supernovae

Jade Powell, Bernhard Müller, Alexander Heger

We present 3D core-collapse supernova simulations of massive Pop-III progenitor stars at the transition to the pulsational pair instability regime. We simulate two progenitor model…

astro-ph.GA2021

On the Evolution of Supermassive Primordial Stars in Cosmological Flows

Tyrone E. Woods, Samuel Patrick, Jacob S. Elford +2

Primordial supermassive stars (SMSs) formed in atomic-cooling halos at z ~ 15 - 20 are leading candidates for the seeds of the first quasars. Past numerical studies of the evolutio…