Radio Detection of SN 1986E in NGC 4302
M. J. Montes, S. D. Van Dyk, K. W. Weiler, R. A. Sramek, N. Panagia
Abstract
Radio observations of SN 1986E have shown a clear detection of emission at 6 cm wavelength about 8 months after optical discovery. Combined with a number of new upper limits and a study of the possible models, it appears that SN 1986E was probably a fairly normal Type IIL supernova, somewhat similar to SN 1980K, with radio emission at roughly expected levels. This detection continues the correlation between radio detection and late time optical emission.
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