Published in
Oxford University Press (OUP), Monthly Notices of the Royal Astronomical Society: Letters, 1(464), p. L65-L69
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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
Journal article published in 2016 by
Wynn C. G. Ho 
,
Nils Andersson
,
Nils Andersson
This paper was not found in any repository, but could be made available legally by the author.
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