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Multifrequency Spectral Studies of SNRs

Published online by Cambridge University Press:  25 May 2016

X.Z. Zhang ,
X.J. Wu ,
L.A. Higgs ,
T.L. Landecker ,
D.A. Green  and
D.A. Leahy
X.Z. Zhang
Affiliation:
Beijing Astronomical Observatory, CAS, Beijing 100080, P.R. China
X.J. Wu
Affiliation:
Beijing University, Beijing 100871, P.R. China
L.A. Higgs
Affiliation:
DRAO, P.O. Box 248, Penticton, B.C. V2A 6K3, Canada
T.L. Landecker
Affiliation:
DRAO, P.O. Box 248, Penticton, B.C. V2A 6K3, Canada
D.A. Green
Affiliation:
MRAO, Cambridge CB3 0HE, UK
D.A. Leahy
Affiliation:
Department of Physics, The University of Calgary, T2N 1N4, Canada

Extract

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Radio supernova remnants(SNRs) of large angular diameter are obvious objects for multifrequency spectral studies from long wavelengths to short wavelengths, as resolutions at low frequency are usually about several arcminutes. An international cooperation consists of MRAO, BAO, DRAO, MPI, and astronomers from Beijing University, Beijing Normal University, China and Calgary University, Canada. This international collaboration is also a part of the Panorramic Spectral Imaging of the Milky Way (PI R. Taylor). Some results on HB21, G78.2+2.1, and HB9 are presented in this paper.

Type
Session 1: Plasma and Fresh Nucleosynthesis Phenomena
Information
Symposium - International Astronomical Union , Volume 188: The Hot Universe , 1998 , pp. 263 - 264
Copyright
Copyright © Kluwer 1998 

References

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