Chirped modulations in the SLSN-I SN 2024afav are modeled as Lense-Thirring precession of an infalling fallback disk around a magnetar, yielding P=4.2 ms and B=1.6e14 G.
inObservational and physical classification of supernovae(eds Alsabti, A
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Lense-Thirring precessing magnetar engine drives a superluminous supernova
Chirped modulations in the SLSN-I SN 2024afav are modeled as Lense-Thirring precession of an infalling fallback disk around a magnetar, yielding P=4.2 ms and B=1.6e14 G.