On the nature of the Supernova Remnant 0540-69.3 in the large Magellanic cloud
| 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.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.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.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 |