most citedRadiatively Cooled Binary Mass Transfer: Flow Structure, Luminosities, and L2 Outflows Across Mass Transfer Rates

1 citations · 1 across the 2 of their papers we have counts for

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9 papers

astro-ph.SR20261 cited

Radiatively Cooled Binary Mass Transfer: Flow Structure, Luminosities, and L2 Outflows Across Mass Transfer Rates

Peter Scherbak, Wenbin Lu, Jim Fuller

High rates of stable mass transfer (MT) occur for some binary star systems, resulting in luminous transients and circumbinary outflows (CBOs). We perform hydrodynamical simulations…

astro-ph.GA2026

Formation of Close Binaries through Massive Black Hole Perturbations and Chaotic Tides

Howard Hao-Tse Huang, Wenbin Lu

Hills breakup of binary systems allows massive black holes (MBH) to produce hyper-velocity stars (HVSs) and tightly bound stars. The long timescale of orbital relaxation means that…

astro-ph.HE2025

A Star's Death by a Thousand Cuts: The Runaway Periodic Eruptions of AT2023uqm

Yibo Wang, Tingui Wang, Shifeng Huang +37

Stars on bound orbits around a supermassive black hole may undergo repeated partial tidal disruption events (rpTDEs), producing periodic flares. While several candidates have been…

astro-ph.SR2025

Rapid binary mass transfer: Circumbinary outflows and angular momentum losses

Peter Scherbak, Wenbin Lu, Jim Fuller

High rates of stable mass transfer likely occur for some binary star systems, but the resulting flow of mass and angular momentum (AM) is unclear. We perform hydrodynamical simulat…

astro-ph.HE2025

Fates of Rotating Supergiants from Stellar Mergers and the Landscape of Transients upon Core-collapse

Daichi Tsuna, Jim Fuller, Wenbin Lu

We present a grid of rotating supergiant models from post-main sequence binary merger products, constructed by the MESA stellar evolution code. We focus on the evolution of these s…

astro-ph.HE2025

Accretion from a shock-inflated companion: double-peaked supernova lightcurve with periodic modulations

Wenbin Lu, Savannah Cary, Daichi Tsuna

We study the observational signatures from the interactions between a newly born neutron star and a companion star that is impacted by the supernova ejecta. We focus on the cases w…