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