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New High Resolution Radio Observations of 3C10, 3C58 and Part of the Cygnus Loop

Published online by Cambridge University Press:  04 August 2017

D. A. Green  and
S. F. Gull
D. A. Green
Affiliation:
Mullard Radio Astronomy Observatory, Cavendish Laboratory, Cambridge, United Kingdom.
S. F. Gull
Affiliation:
Mullard Radio Astronomy Observatory, Cavendish Laboratory, Cambridge, United Kingdom.

Extract

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We present new high resolution observations of 3C10 (Tycho's SN) and 3C58, made at 2.7 GHz with the Cambridge 5 km telescope. These observations have a resolution of ∼ 4 arcsec, considerably better than previous observations, giving a detailed view of the radio morphology of these two remnants. These maps have also been processed by the Maximum Entropy Method (MEM).

Type
III. Center Filled Morphologies
Information
Symposium - International Astronomical Union , Volume 101: Supernova Remnants and Their X-Ray Emission , 1983 , pp. 329 - 334
Copyright
Copyright © Reidel 1983 

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