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Consequences of a New Distance Determination of 3C58

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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In this paper we present new observations that show 3C58 is much closer than has been assumed in the past. This necessitates a reappraisal of many of the quantitative comparisons that have been made between 3C58 and the Crab Nebula or other ‘filled-centre’ remnants.

Type
III. Center Filled Morphologies
Information
Symposium - International Astronomical Union , Volume 101: Supernova Remnants and Their X-Ray Emission , 1983 , pp. 335 - 340
Copyright
Copyright © Reidel 1983 

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