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Australia Telescope observations of the supernova remnant N49 in the LMC

Published online by Cambridge University Press:  19 July 2016

Norbert Junkes
Norbert Junkes*
Affiliation:
Australia Telescope National Facility† Epping, NSW, 2121, Australia

Abstract

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We present the first high-resolution radio image of the supernova remnant N49 near the northern edge of the LMC. These observations with the Australia Telescope at 6cm wavelength (4 arcsec resolution) show a distinct radio shell. The shell structure of N49 is similar in radio and X-ray emission, with the maximum of the emission found in the southeastern part of the SNR.

Type
Stellar Evolution
Information
Symposium - International Astronomical Union , Volume 148: The Magellanic Clouds , 1991 , pp. 347 - 348
Copyright
Copyright © Kluwer 1991 

References

Helfand, D.J. & Long, K.S.: (1979), Nature 282, 589.Google Scholar
Henize, K.G.: (1956), Astrophys. J. Suppl. 2, 315.Google Scholar
Mathewson, D.S., Ford, V.L., Dopita, M.A., Tuohy, I.R., Long, K.S. & Helfand, D.J.: (1983), Astrophys. J. Suppl. 51, 345.Google Scholar
Milne, D.K., Caswell, J.L. & Haynes, R.F.: (1980), Mon. Not. R. astron. Soc. 191, 469.Google Scholar
Shull, P., Dyson, J.E., Kahn, F.D. & West, K.A.: (1985), Mon. Not. R. astron. Soc. 212, 799.Google Scholar