Showing 1–20 of 34 results
/ Date/ Name
Feb 12, 2018A fallback accretion model for the unusual type II-P supernova iPTF14hlsAug 19, 2016Solving the 56Ni puzzle of magnetar-powered broad-lined type Ic supernovaeJun 1, 2022iPTF14hls in the circumstellar medium interaction model: A promising candidate for a pulsational pair-instability supernovaSep 26, 2019CDF-S XT1 and XT2: White Dwarf Tidal Disruption Events by Intermediate-Mass Black Holes?Nov 16, 2010Recovering modified Newtonian dynamics by changing inertiaFeb 10, 2017A Monte Carlo approach to magnetar-powered transients: II. Broad-lined type Ic supernovae not associated with GRBsJul 26, 2017Modeling The Most Luminous Supernova Associated with a Gamma-Ray Burst, SN 2011klSep 13, 2018Photospheric Radius Evolution of Homologous ExplosionsApr 12, 2022A Study on the X-Ray Pulse Profile and Spectrum of the Crab Pulsar Using NICER and Insight-HXMT's ObservationsFeb 20, 2018A Multiple Ejecta-Circumstellar Medium Interaction Model and Its Implications for Superluminous Supernovae iPTF15esb and iPTF13dccSep 22, 2020A Reader Friendly Formalism for Circumstellar Material-Supernova Ejecta Interaction ModelMay 26, 2023A spectral-timing study of the inner flow geometry in MAXI J1535--571 with $Insight$-HXMT and NICERJun 6, 2017A Multiple Ejecta-Circumstellar Meduim Interaction Model and Its Implications for the Superluminous Supernova iPTF15esbMar 2, 2023Insight-HXMT and GECAM-C observations of the brightest-of-all-time GRB 221009AJun 4, 2023Spectral and Jet Properties of the Quasi-thermal Dominated GRB 210121A, GRB 210610B and GRB 221022BSep 22, 2020Discovery of oscillations above 200 keV in a black hole X-ray binary with Insight-HXMTDec 12, 2011Regularity of traveling free surface water waves with vorticityMay 17, 2017A Monte Carlo Approach to Magnetar-powered Transients: I. Hydrogen-deficient Superluminous SupernovaeDec 7, 2018Observations of SN 2017ein Reveal Shock Breakout Emission and A Massive Progenitor Star for a Type Ic SupernovaMar 19, 2020The braking index of PSR B0540-69 and the associated pulsar wind nebula emission after spin-down rate transition