A coupled magnetar–CSM hybrid model produces diverse SLSN light curves by letting the magnetar-driven shock overtake and dominate circumstellar interaction.
@doi [ ] 10.1088/0004-637X/746/2/130, http://adsabs.harvard.edu/abs/2012ApJ...746..130H 746
4 Pith papers cite this work, alongside 195 external citations. Polarity classification is still indexing.
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Core-collapse supernova models including C-O shell mergers best match observed elemental ratios in Cas A, indicating mergers occur and contribute up to 20-30% of 44Ti outside the reverse shock.
Hydrodynamic simulations of three pairs of jittering jets in a CCSN reproduce the ring-and-bar morphology of SNR G11.2-0.3.
Thin-shell numerical model of supernova remnants shows high ambient densities inhibit the Sedov-Taylor phase and prevent the reverse shock from reaching the explosion center above n0 = 5e5 cm^-3 due to rapid cooling.
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A Magnetar Engine and Circumstellar Medium Interaction: Synergistic Effects in Producing Superluminous Supernovae
A coupled magnetar–CSM hybrid model produces diverse SLSN light curves by letting the magnetar-driven shock overtake and dominate circumstellar interaction.
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Production of heavy $\alpha$-elements and $^{44}$Ti in Cas A: comparison to abundances from 1D core-collapse supernova models and evidence for Carbon-Oxygen shell mergers
Core-collapse supernova models including C-O shell mergers best match observed elemental ratios in Cas A, indicating mergers occur and contribute up to 20-30% of 44Ti outside the reverse shock.
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Reproducing morphological features in the supernova remnant G11.2-0.3 by simulating jittering jets
Hydrodynamic simulations of three pairs of jittering jets in a CCSN reproduce the ring-and-bar morphology of SNR G11.2-0.3.
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The full evolution of supernova remnants in low and high density ambient media
Thin-shell numerical model of supernova remnants shows high ambient densities inhibit the Sedov-Taylor phase and prevent the reverse shock from reaching the explosion center above n0 = 5e5 cm^-3 due to rapid cooling.