Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/4272
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dc.contributor.authorRadhakrishnan, V.-
dc.contributor.authorCooke, D.J.-
dc.contributor.authorKomesaroff, M.M.-
dc.contributor.authorMorris, D.-
dc.date.accessioned2012-01-17T10:04:13Z-
dc.date.available2012-01-17T10:04:13Z-
dc.date.issued1969-02-
dc.identifier.citationNature, 1969, Vol. 221, p443-446en
dc.identifier.issn0028-0836-
dc.identifier.issn1476-4687 (Online)-
dc.identifier.urihttp://hdl.handle.net/2289/4272-
dc.descriptionRestricted Access.en
dc.language.isoenen
dc.publisherNature Publishing Groupen
dc.relation.urihttp://adsabs.harvard.edu/abs/1969Natur.221..443Ren
dc.relation.urihttp://dx.doi.org/10.1038/221443a0en
dc.rights1969 Nature Publishing Groupen
dc.titleEvidence in support of a rotational model for the pulsar PSR 0833-45en
dc.typeArticleen
Appears in Collections:Research Papers (A&A)

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