activity
19952020
most citedRossby Wave Instability of Keplerian Accretion Disks

621 citations · 1.6k across the 14 of their papers we have counts for

collaborators

14 papers

astro-ph.EP2020★ 32 cited

Planet-induced Vortices with Dust Coagulation in Protoplanetary Disks

Ya-Ping Li, Hui Li, Shengtai Li +3

In this work, we study how the dust coagulation/fragmentation will influence the evolution and observational appearances of vortices induced by a massive planet embedded in a low v…

astro-ph.EP2019★ 21 cited

Effects of Ringed Structures and Dust Size Growth on Millimeter Observations of Protoplanetary Disks

Ya-Ping Li, Hui Li, Luca Ricci +7

The growth of solids from sub-micron to millimeter and centimeter sizes is the early step toward the formation of planets inside protoplanetary disks (PPDs). However, such processe…

astro-ph.HE2018★ 153 cited

Very high energy particle acceleration powered by the jets of the microquasar SS 433

HAWC Collaboration, A. U. Abeysekara, A. Albert +104

SS 433 is a binary system containing a supergiant star that is overflowing its Roche lobe with matter accreting onto a compact object (either a black hole or neutron star). Two jet…

physics.plasm-ph2018★ 26 cited

Strongly localized magnetic reconnection by the super-Alfvenic shear flow

Yi-Hsin Liu, Michael Hesse, Fan Guo +2

We demonstrate the dragging of the magnetic field by the super-Alfvenic shear flows out of the reconnection plane can strongly localize the reconnection x-line in collisionless pla…

astro-ph.HE2017★ 12 cited

Magnetized Reverse Shock: Density-fluctuation-induced Field Distortion, Polarization Degree Reduction, and Application to GRBs

Wei Deng, Bing Zhang, Hui Li +1

The early optical afterglow emission of several gamma-ray bursts (GRBs) shows a high linear polarization degree (PD) of tens of percent, suggesting an ordered magnetic field in the…

physics.plasm-ph2014★ 43 cited

Energy dynamics and current sheet structure in fluid and kinetic simulations of decaying magnetohydrodynamic turbulence

K. D. Makwana, V. Zhdankin, H. Li +2

Simulations of decaying magnetohydrodynamic (MHD) turbulence are performed with a fluid and a kinetic code. The initial condition is an ensemble of long-wavelength, counter-propaga…