Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/1062
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dc.contributor.authorSrinivasan, G.-
dc.contributor.authorBhattacharya, D.-
dc.date.accessioned2006-01-03T06:15:05Z-
dc.date.available2006-01-03T06:15:05Z-
dc.date.issued1984-05-20-
dc.identifier.citationCurrent Science, 1984, Vol. 53, p513 -516.en
dc.identifier.issn0011-3891-
dc.identifier.urihttp://hdl.handle.net/2289/1062-
dc.description.abstractThe implications of the recently discovered x-ray pulsar within the SNR 054069.3 in the Large Magellanic Cloud is investigated. It is suggested that the SNR is a.shell-plerion combination.en
dc.format.extent301372 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.titleOn the nature of the Supernova Remnant 0540-69.3 in the large Magellanic clouden
dc.typeArticleen
Appears in Collections:Research Papers (A&A)

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