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19972023
most citedPhysics of Strongly Magnetized Neutron Stars

833 citations · 2.5k across the 49 of their papers we have counts for

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6 papers · 1 filter

astro-ph.SR2020

3D MHD Simulations of Accretion onto Stars with Tilted Magnetic and Rotational Axes

M. M. Romanova, A. V. Koldoba, G. V. Ustyugova +3

We present results of global three-dimensional (3D) magnetohydrodynamic (MHD) simulations of accretion onto magnetized stars where both the magnetic and rotational axes of the star…

astro-ph.SR20207 cited

Excitation of Spin-Orbit Misalignments in Stellar Binaries with Circumbinary Disks: Application to DI Herculis

Kassandra R. Anderson, Dong Lai

The large spin-orbit misalignments in the DI Herculis stellar binary system have resolved the decades-long puzzle of the anomalously slow apsidal precession rate, but raise new que…

astro-ph.SR2019

Tidal Evolution of Eccentric Binaries Driven by Convective Turbulent Viscosity

Michelle Vick, Dong Lai

Tidal dissipation due to convective turbulent viscosity shapes the evolution of a variety of astrophysical binaries. For example, this type of dissipation determines the rate of or…

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.SR201537 cited

Electromagnetic Torques, Precession and Evolution of Magnetic Inclination of Pulsars

J. J. Zanazzi, Dong Lai

We present analytic calculations of the electromagnetic torques acting on a magnetic neutron star rotating in vacuum, including near-zone torques associated with the inertia of dip…

astro-ph.SR201016 cited

Low- instabilities in differentially rotating proto-neutron stars with magnetic fields

Wen Fu, Dong Lai

Recent hydrodynamical simulations have shown that differentially rotating neutron stars formed in core-collapse supernovae may develop global non-axisymmetric instabilities even wh…