activity
20102022
most citedMagnetic effect on dynamical tide in rapidly rotating astronomical objects

29 citations · 170 across the 25 of their papers we have counts for

collaborators

25 papers

astro-ph.SR2022★ 11 cited

Magnetic effect on equilibrium tides and its influence on the orbital evolution of binary systems

Xing Wei

In the standard theory of equilibrium tides, hydrodynamic turbulence is considered. In this paper we study the effect of magnetic fields on equilibrium tides. We find that the turb…

astro-ph.SR2022★ 3 cited

Tidal dynamo in solar-like close binary stars

Xing Wei

Thermal convection is commonly believed to be the energy source of stellar or planetary dynamo. In this short paper we provide another possibility, namely large-scale tidal flow. I…

astro-ph.EP2022★ 8 cited

Why hot Jupiters can be large but not too large

Qiang Hou, Xing Wei

Tidal heating is often used to interpret "radius anomaly" of hot Jupiters (i.e. radii of a large fraction of hot Jupiters are in excess of 1.2 Jupiter radius which cannot be interp…

astro-ph.SR2022★ 6 cited

Estimations and scaling laws for stellar magnetic fields

Xing Wei

In rapidly rotating turbulence (Rossby number much less than unity), the standard mixing length theory for turbulent convection breaks and Coriolis force enters the force balance s…

astro-ph.SR2021★ 3 cited

Convectively coupled equatorial trapped waves in stars and planets

Tao Cai, Cong Yu, Xing Wei

In this paper, we have studied the convectively coupled equatorially trapped waves in rotating stars, with and without magnetic field. The equatorial trapped HD and MHD Poincaré, R…

physics.flu-dyn2021★ 4 cited

Enhancement of wave transmissions in multiple radiative and convective zones

Tao Cai, Cong Yu, Xing Wei

In this paper, we study wave transmission in a rotating fluid with multiple alternating convectively stable and unstable layers. We have discussed wave transmissions in two differe…