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Ejector and propeller spin-down: how might a superluminous supernova millisecond magnetar become the 6.67 h pulsar in RCW 103 (2017)

First Author: Ho W

Attributed to: General Relativistic Astrophysics funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.1093/mnrasl/slw186

Publication URI: http://dx.doi.org/10.1093/mnrasl/slw186

Type: Journal Article/Review

Parent Publication: Monthly Notices of the Royal Astronomical Society: Letters

Issue: 1