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http://hdl.handle.net/2289/875| Title: | On the implications of the radio and x-ray pulsar in the supernova remnant MSH 15-52 |
| Authors: | Srinivasan, G. Dwarakanath, K.S. Radhakrishnan, V. |
| Issue Date: | 20-Jun-1982 |
| Publisher: | Indian Academy of Sciences, Bangalore, India. |
| Citation: | Current Science, 1982, Vol. 51, p596-599. |
| Abstract: | Comparison of the X-ray nebulosity surrounding the X-ray and radio pulsar in the shell-type SNR MSH 15-52 with the Crab nebula leads to an initial period for the pulsar ~ 70 ms. The association of the pulsar with the shell remnant confirms the validity of the ∑-t approach in determining the ages of young SNRs using historical calibrators. |
| URI: | http://hdl.handle.net/2289/875 |
| ISSN: | 0011-3891 |
| Copyright: | Indian Academy of Sciences, Bangalore, India. |
| Appears in Collections: | Research Papers (A&A) |
Files in This Item:
| File | Description | Size | Format | |
|---|---|---|---|---|
| 1982 CS V51 p596.pdf | 4p. | 281.83 kB | Adobe PDF | View/Open |
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