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Aperture Synthesis Observations of the Supernova Remnant G73.9+0.9
Published online by Cambridge University Press: 12 April 2016
Abstract
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Radio continuum observations, obtained with the DRAO Synthesis Telescope, are presented of the new supernova remnant (SNR) G73.9+0.9. Our map at 1420 MHz shows indications of spatially resolved knots of emission in the brightest part of the remnant. The 408 MHz map, although of lower resolution, shows the same general morphology. The spectral index α (Sv∝v−α) between 1420 and 408 MHz is about 0.5, a value typical for shell type SNRs. The morphology however is more suggestive of a filled centre SNR.
- Type
- Research Article
- Information
- International Astronomical Union Colloquium , Volume 101: Supernova Remnants and the Interstellar Medium , 1988 , pp. 297 - 300
- Copyright
- Copyright © Cambridge University Press 1988
References
Haslam, C.G.T., Salter, C.J., Stoffel, H., and Wilson, W.E.: 1982, Astron. Astrophys. Suppl., 47, 1
Google Scholar
Reich, W., Fürst, E., Reich, P., Sofue, Y., and Handa, T.: 1986, Astron. Astrophys.
155, 185–192
Google Scholar
Roger, R.S., Costain, C.H., Lacey, J.D., Landecker, T.L., and Bowers, F.K.: 1973, Proc. IEEE, 61, 1270
Google Scholar
Weiler, K.W.: 1984, in Supernova Remnants and their X-ray emission, IAU Symp. No. 101, eds. Danziger, I., Gorenstein, P., D. Reidel, Dordrecht, p. 299
Google Scholar
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