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A high-resolution radio survey of the Vela supernova remnant | | D. C.-J. Bock
; A. J. Turtle
; A. J. Green
; | | Date: |
13 Jul 1998 | | Journal: | Astron.J. 116 (1998) 1886 | | Subject: | astro-ph | | Abstract: | This paper presents a high-resolution radio continuum (843 MHz) survey of the Vela supernova remnant. The contrast between the structures in the central pulsar-powered nebula of the remnant and the synchrotron radiation shell allows the remnant to be identified morphologically as a member of the composite class. The data are the first of a composite remnant at spatial scales comparable with those available for the Cygnus Loop and the Crab Nebula, and make possible a comparison of radio, optical and soft X-ray emission from the resolved shell filaments. The survey, made with the Molonglo Observatory Synthesis Telescope, covers an area of 50 square degrees at a resolution of 43’’ x 60’’, while imaging structures on scales up to 30’. | | Source: | arXiv, astro-ph/9807125 | | Services: | Forum | Review | PDF | Favorites | |
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