Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/2396
Full metadata record
DC FieldValueLanguage
dc.contributor.authorBhattacharya, D.-
dc.date.accessioned2007-05-25T07:55:47Z-
dc.date.available2007-05-25T07:55:47Z-
dc.date.issued1992-
dc.identifier.citationIAU Colloquium, 1992, Vol.128, p27en
dc.identifier.urihttp://hdl.handle.net/2289/2396-
dc.descriptionRestricted Access. Magnetospheric Structure and Emission Mechanics of Radio Pulsars, Proceedings of IAU Colloq. 128, held in Lagow, Poland, 17-22 June 1990. Edited by T. H. Hankins, J. M. Rankin, and J. A. Gil. Pedagogical Univ. Press, 1992en
dc.format.extent599334 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherPedagogical University Pressen
dc.relation.urihttp://adsabs.harvard.edu/cgi-bin/bib_query?1992msem.coll...27Ben
dc.rights1992 Pedagogical University Pressen
dc.titleThe evolution of the magnetic fields of neutron starsen
dc.typeArticleen
Appears in Collections:Research Papers (A&A)

Files in This Item:
File Description SizeFormat 
1992 IAU COLL V128 p27.pdf
  Restricted Access
Restricted Access585.29 kBAdobe PDFView/Open Request a copy


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