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A Suspected Supernova in A.D. 1181

Published online by Cambridge University Press:  08 February 2017

F.R. Stephenson
F.R. Stephenson*
Affiliation:
Department of Geophysics and Planetary Physics, School of Physics, University of Newcastle upon Tyne

Summary

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The new star which appeared in Cassiopeia in A.D. 1181 attracted considerable attention in the Far East. It was visible for about six months, and its position was carefully recorded by the Chinese and Japanese astronomers. Their observational evidence favours the identification of the star as a supernova of type I. It is proposed that the radio source 3C 58 is the remnant of the new star.

Information

Type
Research Article
Information
International Astronomical Union Colloquium , Volume 8: Experimental Techniques for the Determination of Fundamental Spectroscopic Data , March 1971 , pp. 10 - 38
Copyright
Copyright © Blackwell Scientific Publications 1971

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