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http://hdl.handle.net/2289/1062
Full metadata record
DC Field | Value | Language |
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dc.contributor.author | Srinivasan, G. | - |
dc.contributor.author | Bhattacharya, D. | - |
dc.date.accessioned | 2006-01-03T06:15:05Z | - |
dc.date.available | 2006-01-03T06:15:05Z | - |
dc.date.issued | 1984-05-20 | - |
dc.identifier.citation | Current Science, 1984, Vol. 53, p513 -516. | en |
dc.identifier.issn | 0011-3891 | - |
dc.identifier.uri | http://hdl.handle.net/2289/1062 | - |
dc.description.abstract | The 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.extent | 301372 bytes | - |
dc.format.mimetype | application/pdf | - |
dc.language.iso | en | en |
dc.publisher | Indian Academy of Sciences, Bangalore, India. | en |
dc.rights | Indian Academy of Sciences, Bangalore, India. | en |
dc.title | On the nature of the Supernova Remnant 0540-69.3 in the large Magellanic cloud | en |
dc.type | Article | en |
Appears in Collections: | Research Papers (A&A) |
Files in This Item:
File | Description | Size | Format | |
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1984 CS V53 p513.pdf | 4p. | 294.31 kB | Adobe PDF | View/Open |
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