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Rotational evolution of young pulsars due to superfluid decoupling

Rotational evolution of young pulsars due to superfluid decoupling
Rotational evolution of young pulsars due to superfluid decoupling
1745-2473
787-789
Ho, Wynn C.G.
d78d4c52-8f92-4846-876f-e04a8f803a45
Andersson, Nils
2dd6d1ee-cefd-478a-b1ac-e6feedafe304
Ho, Wynn C.G.
d78d4c52-8f92-4846-876f-e04a8f803a45
Andersson, Nils
2dd6d1ee-cefd-478a-b1ac-e6feedafe304

Ho, Wynn C.G. and Andersson, Nils (2012) Rotational evolution of young pulsars due to superfluid decoupling. Nature Physics, 8, 787-789. (doi:10.1038/nphys2424).

Record type: Article

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More information

Published date: 30 September 2012
Organisations: Applied Mathematics

Identifiers

Local EPrints ID: 339209
URI: http://eprints.soton.ac.uk/id/eprint/339209
ISSN: 1745-2473
PURE UUID: 85a5e8dc-3bc9-4570-995b-90e068981a4d
ORCID for Wynn C.G. Ho: ORCID iD orcid.org/0000-0002-6089-6836
ORCID for Nils Andersson: ORCID iD orcid.org/0000-0001-8550-3843

Catalogue record

Date deposited: 25 May 2012 08:40
Last modified: 15 Mar 2024 02:59

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