Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/3382
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dc.contributor.advisorSrinivasan, G.-
dc.contributor.authorJahan Miri, M.-
dc.date.accessioned2008-01-17T09:47:13Z-
dc.date.available2008-01-17T09:47:13Z-
dc.date.issued1996-
dc.identifier.citationPh.D. Thesis, Indian Institute of Science, Bangalore, 1996.en
dc.identifier.urihttp://hdl.handle.net/2289/3382-
dc.descriptionOpen Accessen
dc.format.extent378311 bytes-
dc.format.extent1358128 bytes-
dc.format.extent2915352 bytes-
dc.format.extent2407807 bytes-
dc.format.extent1802961 bytes-
dc.format.extent430052 bytes-
dc.format.mimetypeapplication/pdf-
dc.format.mimetypeapplication/pdf-
dc.format.mimetypeapplication/pdf-
dc.format.mimetypeapplication/pdf-
dc.format.mimetypeapplication/pdf-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherRaman Research Institue, Bangalore.en
dc.rightsThis thesis is posted here with the permission of the author. Personal use of this material is permitted. Any other use requires prior permission of the author. By choosing to view this document, you agree to all provisions of the copyright laws protecting it.en
dc.subject.classificationAstronomy and Astrophysicsen
dc.titleThe evolution of the magnetic fields of neutron stars : The role of the superfluid states in their interiors.en
dc.typeThesisen
Appears in Collections:Theses (A&A)

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Chapter 5 & 6.pdfOpen Access158.76 kBAdobe PDFView/Open
Chapter 4.pdfOpen Access620.59 kBAdobe PDFView/Open
Chapter 3.pdfOpen Access889.98 kBAdobe PDFView/Open
Chapter 2.pdfOpen Access1.07 MBAdobe PDFView/Open
Chapter 1.pdfOpen Access573.45 kBAdobe PDFView/Open
Title, Contents etc..pdfOpen Access107.76 kBAdobe PDFView/Open


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