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Deceleration in the Expansion of SN 1993J
Published online by Cambridge University Press: 12 April 2016
Abstract
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With new 6 cm observations we confirm the self-similar expansion of SN 1993J previously discovered at 3.6 cm and estimate the expansion deceleration parameter. The results are inconsistent with the existence of a constant pre-explosion stellar wind but otherwise confirm the standard radio supernova model. The first map at 13 cm showing shell structure is also presented.
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- Research Article
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- Copyright
- Copyright © Astronomical Society of the Pacific 1998
References
Chevalier, R.A.
1996. in Radio Emission from the Stars and the Sun, eds. Taylor, A.R., & Paredes, J.M. (San Francisco: ASP Conference Series, Vol. 93), 125–133.Google Scholar
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