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High-Resolution Observations of Galactic Nonthermal Sources at 160 Mhz
Published online by Cambridge University Press: 14 August 2015
Abstract
Preliminary maps of the brightness distributions of 11 supernova remnants are presented. The sources, with diameters ≲10′, were observed at 160 MHz with resolution better than 2′. Ten of the supernova remnants are significantly resolved, and at least six show evidence of a shell-like structure. For those sources where high-frequency maps are available with comparable resolution the brightness distributions are generally very similar.
- Type
- Part 3: Supernova Remnants
- Information
- Symposium - International Astronomical Union , Volume 60: Galactic Radio Astronomy , 1974 , pp. 347 - 351
- Copyright
- Copyright © Reidel 1974
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