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The Kinematics of The SNR G292.0+1.8

Published online by Cambridge University Press:  04 August 2017

R. Braun ,
W. M. Goss ,
I. J. Danziger  and
A. Boksenberg
R. Braun
Affiliation:
Sterrewacht Leiden, The Netherlands
W. M. Goss
Affiliation:
Kapteyn Astronomical Institute, Groningen, The Netherlands
I. J. Danziger
Affiliation:
European Southern Observatory, Garching bei München, F.R.G.
A. Boksenberg
Affiliation:
Royal Greenwich Observatory, Herstmonceux Castle, Hailsham, U.K.

Abstract

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Optical velocity field mapping of G292.0+1.8 in the [0III] λ5007 å line has been carried out using the IPCS with the 3.6 m ESO telescope at La Silla. Our data are not consistent with the suggestion that the [0III] emitting material in the western portion of this remnant is concentrated in an expanding ring. The existing data on G292.0+1.8 suggests that only the brightest portion of a thick shell of ejecta with high velocity spurs is observed. The expansion centroid, size, velocity and age of this SNR are derived.

Type
I. Young Supernova Remnants
Information
Symposium - International Astronomical Union , Volume 101: Supernova Remnants and Their X-Ray Emission , 1983 , pp. 159 - 164
Copyright
Copyright © Reidel 1983 

References

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