Low-frequency observations of the Vela supernova remnant  and their implications

Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/745

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DC Field	Value	Language
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.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.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.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
Appears in Collections:	Research Papers (A&A)

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