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Comparison of Radio and X-ray Observations of SNR G109.1–1.0

Published online by Cambridge University Press:  04 August 2017

P. C. Gregory ,
R. Braun ,
G. G. Fahlman  and
S. F. Gull
P. C. Gregory
Affiliation:
Department of Physics, University of British Columbia, Vancouver, Canada
R. Braun*
Affiliation:
Department of Physics, University of British Columbia, Vancouver, Canada
G. G. Fahlman
Affiliation:
Department of Geophysics and Astronomy, University of British Columbia, Vancouver, Canada
S. F. Gull
Affiliation:
Mullard Radio Astronomy Observatory, Cambridge University, Cambridge, U.K.
*
Sterrenwacht Leiden

Extract

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In this paper, we present a comparison of the radio and X-ray morphology of the supernova remnant G109.1–1.0, based on recent radio observations at 6 and 20 cm and investigate the relationship of the SNR to a neighbouring molecular cloud.

Type
V. Compact Objects Associated With Supernova Remnants, Pulsars and Neutron Stars
Information
Symposium - International Astronomical Union , Volume 101: Supernova Remnants and Their X-Ray Emission , 1983 , pp. 437 - 443
Copyright
Copyright © Reidel 1983 

References

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