1. RRI Digital Repository
  2. 04. Astronomy and Astrophysics
  3. Research Papers (A&A)
Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/1078
Full metadata record
DC FieldValueLanguage
dc.contributor.authorBhattacharya, D.-
dc.contributor.authorShukre, C.S.-
dc.date.accessioned2006-01-04T05:43:51Z-
dc.date.available2006-01-04T05:43:51Z-
dc.date.issued1985-
dc.identifier.citationJournal of Astrophysics and Astronomy, 1985, Vol. 6, p233-237.en
dc.identifier.issn0250-6335-
dc.identifier.urihttp://hdl.handle.net/2289/1078-
dc.description.abstractThe evolution of rotation period and spindown age of a pulsar whose surface magnetic field undergoes a phase of growth were investigated. Application of these results to the Crab pulsar strongly indicates that its parameters cannot be accounted for by the field growth theories.en
dc.format.extent490069 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherIndian Academy of Sciences, Bangalore, India.en
dc.rightsIndian Academy of Sciences, Bangalore, India.en
dc.subjectPulsarsen
dc.subjectMagnetic fielden
dc.subjectEvolution - Pulsarsen
dc.titleHas the Crab Pulsar magnetic field grown after its birth?en
dc.typeArticleen
Appears in Collections:Research Papers (A&A)

Files in This Item:
File Description SizeFormat 
1985_JAA_V6_p233-237.pdf5p.478.58 kBAdobe PDFView/Open
Show simple item record


Items in RRI Digital Repository are protected by copyright, with all rights reserved, unless otherwise indicated.