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19972022
most citedPhysics of Strongly Magnetized Neutron Stars

833 citations · 2.5k across the 45 of their papers we have counts for

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Showing 2018Show all

8 papers · 1 filter

astro-ph.SR201810 cited

Polygram Stars: Resonant Tidal Excitation of Fundamental Oscillation Modes in Asynchronous Stellar Coalescence

Morgan MacLeod, Michelle Vick, Dong Lai +1

The prevalence of binary stars at close separations implies that many of these systems will interact or merge during the binary's lifetime. This paper presents hydrodynamic simulat…

astro-ph.EP201884 cited

Chaotic Tides in Migrating Gas Giants: Forming Hot and Transient Warm Jupiters via High-Eccentricity Migration

Michelle Vick, Dong Lai, Kassandra R. Anderson

High-eccentricity migration is an important channel for the formation of hot Jupiters (HJs). In particular, Lidov-Kozai (LK) oscillations of orbital eccentricity/inclination induce…

astro-ph.HE2018

Hydrodynamics of circumbinary accretion: Angular momentum transfer and binary orbital evolution

Diego J. Muñoz, Ryan Miranda, Dong Lai

We carry out 2D viscous hydrodynamical simulations of circumbinary accretion using the AREPO code. We self-consistently compute the accretion flow over a wide range of spatial scal…

astro-ph.HE2018

Enhanced Black-Hole Mergers in Binary-Binary Interactions

Bin Liu, Dong Lai

We study the orbital evolution of black hole (BH) binaries in quadruple systems, where the tertiary binary excites large eccentricity in the BH binary through Lidov-Kozai (LK) osci…

astro-ph.EP2018

Teetering Stars: Resonant Excitation of Stellar Obliquities by Hot and Warm Jupiters with External Companions

Kassandra R. Anderson, Dong Lai

Stellar spin-orbit misalignments (obliquities) in hot Jupiter systems have been extensively probed. Such obliquities may reveal clues about hot Jupiter dynamical histories. Common…

astro-ph.EP2018

Photoevaporation and High-Eccentricity Migration Created the Sub-Jovian Desert

James E. Owen, Dong Lai

The mass-period or radius-period distribution of close-in exoplanets shows a paucity of intermediate mass/size (sub-Jovian) planets with periods ~< 3 days. We show that this sub-Jo…