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20232026
most citedBinary mass transfer in 3D: Mass Transfer Rate and Morphology

8 citations · 15 across the 11 of their papers we have counts for

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7 papers · 1 filter

astro-ph.SR20264 cited

Thermal-timescale accretion does not always yield critical rotation in mass gainers

Chen Wang, Mike Y. M. Lau, Xiang-Dong Li +7

Binary evolution plays a central role in producing rapidly rotating stars. Previous studies have shown that mass gainers in binaries can reach critical rotation after accreting onl…

astro-ph.SR2025

AREPO-RSG: Aspherical Circumstellar Material and Winds from Pulsating Dusty Red Supergiants in Global 3D Radiation Hydrodynamic Simulations

Jing-Ze Ma, Stephen Justham, Ruediger Pakmor +3

Recent observations have revealed a surprisingly large fraction of hydrogen-rich supernovae (SNe) interacting with dense confined circumstellar material (CSM), whose origin is heav…

astro-ph.SR2025

The collision and merger products of stars do not look alike: A magnetohydrodynamics comparison

Pavan Vynatheya, Taeho Ryu, Chen Wang +2

A significant fraction of stars experience close interactions, including collisions resulting from gravitational encounters and mergers within close binary systems. These processes…

astro-ph.SR20258 cited

Binary mass transfer in 3D: Mass Transfer Rate and Morphology

T. Ryu, R. Sari, S. E. de Mink +6

Mass transfer is crucial in binary evolution, yet its theoretical treatment has long relied on analytic models whose key assumptions remain debated. We present a direct and systema…

astro-ph.SR20241 cited

Blue straggler stars

Chen Wang, Taeho Ryu

Blue straggler stars are unique main-sequence stars that appear more luminous, hotter, and therefore younger, than their coeval counterparts. In star clusters, these stars are loca…

astro-ph.SR20241 cited

Magnetic Field Amplification during Stellar Collisions between Low-Mass Stars

Taeho Ryu, Alison Sills, Ruediger Pakmor +2

Blue straggler stars in stellar clusters are a subset of stars that are bluer and appear younger than other cluster members, seemingly straggling behind in their evolution. They of…