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Rotational evolution of young pulsars due to superfluid decoupling (2012)

First Author: Ho W

Attributed to: Modelling compact objects for precision astrophysics funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.1038/nphys2424

Publication URI: http://dx.doi.org/10.1038/nphys2424

Type: Journal Article/Review

Parent Publication: Nature Physics

Issue: 11

ISSN: 1745-2473