Fermi-LAT detection of GeV emission from SN 2017egm favors a magnetar central engine over CSM interaction for powering this superluminous supernova.
Title resolution pending
2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
representative citing papers
Magnetized Kerr spacetime admits a critical magnetic field beyond which no circular timelike or null geodesics exist, and subcritical fields induce periastron precession reversal within a finite radial range.
citing papers explorer
-
Gamma-ray signature of superluminous supernovae: Fermi-LAT GeV detection of SN 2017egm and evidence of a central engine
Fermi-LAT detection of GeV emission from SN 2017egm favors a magnetar central engine over CSM interaction for powering this superluminous supernova.
-
Orbital dynamics and precession in magnetized Kerr spacetime
Magnetized Kerr spacetime admits a critical magnetic field beyond which no circular timelike or null geodesics exist, and subcritical fields induce periastron precession reversal within a finite radial range.