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A radiation-hydrodynamics model of accretion columns for ultra-luminous X-ray pulsars
Online Contents | 2016| -
Black Hole Spin Signature in the Black Hole Shadow of M87 in the Flaring State
Free accessArXiv | 2019| -
A Possible Time-Delayed Brightening of the Sgr A* Accretion Flow after the Pericenter Passage of G2 Cloud
Free accessArXiv | 2017| -
A radiation-hydrodynamic model of accretion columns for ultra-luminous X-ray pulsars
Free accessArXiv | 2016| -
Radio Images inside Highly Magnetized Jet Funnels Based on Semi-Analytic GRMHD Models
Free accessArXiv | 2024| -
Polarization images of accretion flow around supermassive black holes: imprints of toroidal field structure
Free accessArXiv | 2020| -
Structure of the super-Eddington outflow and itsimpact on the cosmological scale
Free accessArXiv | 2022| -
Mushroom-instability-driven Magnetic Reconnections in Collisionless Relativistic Jets
Free accessArXiv | 2022|
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