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20242026
most citedPopulation Synthesis Study on the Binary Origin of Type Ibn Supernovae

4 citations · 4 across the 11 of their papers we have counts for

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astro-ph.SR2024

Common envelopes at StanFest

Ilya Mandel, Ryosuke Hirai, Lewis Picker

We describe some of our group's recent work on common envelopes. Our goal is to understand the onset and outcomes of dynamically unstable mass transfer, including the properties of…

astro-ph.SR2024

Evolution of the Convective Core Mass during the Main Sequence

Minori Shikauchi, Ryosuke Hirai, Ilya Mandel

We construct a semi-analytical model that describes the convective core mass evolution of massive stars experiencing mass loss during the main-sequence stage. We first conduct a su…

astro-ph.HE2024

Bumpy Superluminous Supernovae Powered by a Magnetar-star Binary Engine

Jin-Ping Zhu, Liang-Duan Liu, Yun-Wei Yu +4

Wolf-Rayet stars in close binary systems can be tidally spun up by their companions, potentially leaving behind fast-spinning highly-magnetized neutron stars, known as ``magnetars"…

astro-ph.SR2024

Fits for the convective envelope mass in massive stars

Lewis Picker, Ryosuke Hirai, Ilya Mandel

We explore the evolution of massive stars (>8 solar masses) with 1-D models and present analytical fits to the masses and binding energies of the convective portions of their envel…

astro-ph.SR2024

Expansion of accreting main-sequence stars during rapid mass transfer

Mike Y. M. Lau, Ryosuke Hirai, Ilya Mandel +1

Accreting main-sequence stars expand significantly when the mass accretion timescale is much shorter than their thermal timescales. This occurs during mass transfer from an evolved…