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Shell-like Structure in 41.9+58, A Powerful SNR in M82

Published online by Cambridge University Press:  03 August 2017

P. N. Wilkinson  and
A.G. de Bruyn
P. N. Wilkinson
Affiliation:
NRAL, Jodrell Bank, U.K.
A.G. de Bruyn
Affiliation:
NFRA, Dwingeloo, The Netherlands

Extract

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We have studied the brightest of the many compact radio components, designated 41.9+58, in the central region of M82 (Unger et al. 1984; Kronberg et al. 1985) with the EVN at frequencies of 1.6 and 5 GHz (Wilkinson and de Bruyn, 1984; 1987).

Type
Extragalactic
Information
Symposium - International Astronomical Union , Volume 129: The Impact of VLBI on Astrophysics and Geophysics , 1988 , pp. 187 - 188
Copyright
Copyright © Reidel 1988 

References

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