Low-frequency observations of the Vela supernova remnant and their implications
| dc.contributor.author | Dwarakanath, K S | |
| dc.date.accessioned | 2005-12-16T09:30:46Z | |
| dc.date.available | 2005-12-16T09:30:46Z | |
| dc.date.issued | 1991-07-09 | |
| dc.description.abstract | Observations of the Vela SNR at 34.5 MHz are reported and improved spectral-index estimates are presented and discussed. The flux densities of Vela X and YZ at 34.5 MHz are estimated to be 1800 and 3900 Jy, respectively, and their spectral indices are estimated to be -0.16 +/- 0.02 and -0.53 +/- 0.03, respectively. The spectral index estimates, along with other known characteristics, strengthen the hypothesis that Vela X is a plerion, while Vela YZ is a typical shell-type SNR. | en |
| dc.format.extent | 1082166 bytes | |
| dc.format.mimetype | application/pdf | |
| dc.identifier.citation | Journal of Astrophysics and Astronomy, 1991, Vol. 12, p199-211. | en |
| dc.identifier.issn | 0250-6335 | |
| dc.identifier.uri | http://hdl.handle.net/2289/745 | |
| dc.language.iso | en | en |
| dc.publisher | Indian Academy of Sciences, Bangalore, India. | en |
| dc.rights | Indian Academy of Sciences, Bangalore, India. | en |
| dc.subject | Vela supernova remnant | en |
| dc.subject | Vela pulsar | en |
| dc.subject | SNR-PSR association | en |
| dc.title | Low-frequency observations of the Vela supernova remnant and their implications | en |
| dc.type | Article | en |