Ling-Jun Wang
0000-0002-8352-1359
25 papers found
Refreshing results…
The braking index of PSR B0540−69 and the associated pulsar wind nebula emission after spin-down rate transition
CDF-S XT1 and XT2: White Dwarf Tidal Disruption Events by Intermediate-mass Black Holes?
The brightening of the pulsar wind nebula of PSR B0540−69 after its spin-down-rate transition
Broad-lined type Ic supernova iPTF16asu: A challenge to all popular models
Modeling the Light Curves of the Luminous Type Ic Supernova 2007D
The Energy Sources of Superluminous Supernovae
Observations of SN 2017ein Reveal Shock Breakout Emission and a Massive Progenitor Star for a Type Ic Supernova
Photospheric Radius Evolution of Homologous Explosions
A Fallback Accretion Model for the Unusual Type II-P Supernova iPTF14hls
A Multiple Ejecta-circumstellar Medium Interaction Model and Its Implications for Superluminous Supernovae iPTF15esb and iPTF13dcc
A Pulsar Wind Nebula Model Applied to Short GRB 050724
A Monte Carlo Approach to Magnetar-powered Transients. II. Broad-lined Type Ic Supernovae Not Associated with GRBs
Modeling The Most Luminous Supernova Associated with a Gamma-Ray Burst, SN 2011kl
A Monte Carlo Approach to Magnetar-powered Transients. I. Hydrogen-deficient Superluminous Supernovae
Evidence for Magnetar Formation in Broad-lined Type Ic Supernovae1998bw and 2002ap
SOLVING THE56Ni PUZZLE OF MAGNETAR-POWERED BROAD-LINED TYPE IC SUPERNOVAE
A TRIPLE-ENERGY-SOURCE MODEL FOR SUPERLUMINOUS SUPERNOVA iPTF13ehe
Reverse shock emission driven by post-merger millisecond magnetar winds: Effects of the magnetization parameter
Probing the Birth of Post-merger Millisecond Magnetars with X-Ray and Gamma-Ray Emission
Optical Transients Powered by Magnetars: Dynamics, Light Curves, and Transition to the Nebular Phase
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