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

Title: Low-frequency observations of the Vela supernova remnant and their implications
Authors: Dwarakanath, K.S.
Keywords: Vela supernova remnant
Vela pulsar
SNR-PSR association
Issue Date: 9-Jul-1991
Publisher: Indian Academy of Sciences, Bangalore, India.
Citation: Journal of Astrophysics and Astronomy, 1991, Vol. 12, p199-211.
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.
URI: http://hdl.handle.net/2289/745
ISSN: 0250-6335
Copyright: Indian Academy of Sciences, Bangalore, India.
Appears in Collections:Research Papers (A&A)

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