activity
19972026
most citedPresupernova Evolution of Rotating Massive Stars I: Numerical Method and Evolution of the Internal Stellar Structure

1k citations · 5.4k across the 26 of their papers we have counts for

collaborators

23 papers

astro-ph.SR2026

Evolution of wide O star binaries through their LBV stage. Population synthesis with mass-ejection-driven orbital evolution

Xiao-Tian Xu, Philipp Podsiadlowski, Norbert Langer +6

Context. Long-period Wolf-Rayet (WR) star binaries produced by mass transfer are predicted to be abundant, but are observationally rare. This yields constraints on the evolution of…

astro-ph.HE2025★ 2 cited

A solution to the tension of burning on neutron stars and nuclear physics

Y. Cavecchi, D. Galloway, A. Heger +8

When neutron stars accrete matter from a companion star, this matter forms a disc around them and eventually falls on their surface. Here, the fuel can ignite into bright flashes c…

astro-ph.GA2025★ 1 cited

1000-10,000 M Primordial Stars Created the Nitrogen Excess in GS 3073 at

Devesh Nandal, Daniel J. Whalen, Muhammad A. Latif +1

The advent of the James Webb Space Telescope has revealed a wealth of new galaxies just a few hundred Myr after the Big Bang. Some of these galaxies exhibit unusual N/O ratios that…

astro-ph.SR2024

The Impact of Initial Composition on Massive Star Evolution and Nucleosynthesis

Christopher West, Alexander Heger, Benoit Cote +2

We study the sensitivity of presupernova evolution and supernova nucleosynthesis yields of massive stars to variations of the initial composition. We use the solar abundances from…

astro-ph.HE2024

Partial tidal disruption events: The elixir of life

Megha Sharma, Daniel J. Price, Alexander Heger

In our Galactic Center, about 10,000 to 100,000 stars are estimated to have survived tidal disruption events, resulting in partially disrupted remnants. These events occur when a s…

astro-ph.SR2017★ 63 cited

On the Rotation of Supermassive Stars

Lionel Haemmerlé, Tyrone E. Woods, Ralf S. Klessen +2

Supermassive stars born from pristine gas in atomically-cooled haloes are thought to be the progenitors of supermassive black holes at high redshifts. However, the way they accrete…