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High Resolution Radio Observations of the SNR G160.9+2.6 (HB9)

Published online by Cambridge University Press:  12 April 2016

D.A. Leahy  and
R.S. Roger
D.A. Leahy
Affiliation:
Dept. of Physics, University of Calgary, Canada
R.S. Roger
Affiliation:
Dominion Radio Astrophysical Observatory, National Research Council of Canada, Penticton

Abstract

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G160.9+2.6 (HB9) is a supernova remnant of large angular diameter and low radio surface brightness. We report new observations of the continuum emission from HB9 at 408 MHz and 1420 MHz with angular resolutions of 3.5’ and 1.0#x2019;, respectively, which reveal significant filamentary structure not previously detected. The 1420 MHz field covers only the central and eastern parts of HB9. The 408-1420 MHz spectral index (S∝vα) of regions common to both maps is α=-0.68, with no significant spatial variation. The radio filamentary structure closely follows the optical structure. X-ray emission from HB9 is more centrally concentrated than the radio or optical emission. The radio, optical, and particularly, the X-ray surface brightness are all diminished in the northern and northwestern portions of the remnant, in directions approximately coincident with an extensive molecular cloud detected in CO.

Type
Research Article
Information
International Astronomical Union Colloquium , Volume 101: Supernova Remnants and the Interstellar Medium , 1988 , pp. 301 - 304
Copyright
Copyright © Cambridge University Press 1988

References

Dwarakanath, K., Shevgankar, R., and Sastry, C.V. 1982. J. Astrophys. Astr. 3, 207.Google Scholar
Haslam, C.G.T., Salter, C.J., Stoffel, H., and Wilson, W.E. 1982. Astron. Astr. Suppl., 47, 1 Google Scholar
Huang, Y.L. and Thaddeus, P. 1986. Ap. J., 309, 804 Google Scholar
Kallas, E. and Reich, W. 1980, Astron. Astrophys. Suppl.. Ser. 42, 227 Google Scholar
Leahy, D.A. 1987. to appear in Ap. J.Google Scholar
Roger, R.S., Costain, C.H., Lacey, J.D., Landecker, T.L., and Bowers, F.K. 1973. Proc. I.E.E.E., 61, 1270.Google Scholar
Reich, W., Fürst, E., and Selber, W. 1983. IAU Symposium No. 101 “Supernova Remnants and Their X-ray Emission”, Danziger, J., Gorenstein, P. (eds.), (Reidel, Dordrecht), p. 377 Google Scholar
van den Bergh, S., Marscher, A., Terzian, Y. 1973. Ap. J. Suppl., 26, 19.Google Scholar
Veidt, B.G., Landecker, T.L., Vaneldik, J.F., Dewdney, P.E., and Routledge, D. 1985. Radio Science, 20, 237 Google Scholar
Willis, A.G. 1973. Astron. Astrophys. 26, 237.Google Scholar