本所高能天文物理研究方向包括了雙星系統與星系中心流向黑洞吸積之特性,雙星系統中子星及黑洞的形成,從獨立磁化中子星或伽瑪射線雙星系統成員之高能幅射機制。
Image of the Black Hole in M87
Hypernovae and GRB
Localization of a Fast Radio Burst
CASTRO AMR
3D pair-instability supernova model
3D radiation hydrodynamical simulation of Colliding Shells
An exploding supermassive star
Magnetar-powered Superluminous Supernovae
Distribution of the bulk velocity relative to the speed of light
VLBA total intensity map of the M87 jet at 43 GHz (2-a)
Accretion geometry of disks for LLAGN
Accretion geometry of disks for high luminosity AGN
Luminosity evolution of pulsar outer magnetospheric accelerators as a function of neutron star spin down luminosity.
Schematic picture (side view) of a pulsar magnetosphere.
Accretion geometry of disks for LLAGN and high luminosity AGN corresponding to high and low rates of mass accretion respectively.
Prototype of Graphitic Core for Two-Fluid Molten-Salt Heat-Exchanger
Spectral Hardening in the Trailing Peak of Gamma-ray Pulsar Light Curve
Pulsed Gamma-Ray Emission from the Crab Pulsar
Death Line of Gamma-ray Pulsars with Outer Gaps
Monolithic collapse of a weakly magnetized cloud to form black holes