The study of radio emission from SN 1987A after the neutrino burst is reviewed. The observed maximum flux density of the burst at radio wavelengths was about 140 mJy and occurred at 1.4 GHz. The radio light curves for SN 1987A at four frequencies are compared with data for SN 1979C and SN 1980K. VLBI observations of SN 1987A at 2.3 GHz and other radio monitoring programs are examined.
|Original language||English (US)|
|Title of host publication||Supernova 1987A in the Large Magellanic Cloud|
|Subtitle of host publication||Proceedings of the Fourth George Mason Astrophysics Workshop|
|Editors||M. Kafatos, A.G. Michalitsianos|
|Publisher||Cambridge University Press|
|Number of pages||6|
|State||Published - 1988|
- Astronomical Photography, Neutrino Beams, Radio Observation, Supernova 1987a, Australia, H Ii Regions, Photographic Plates, Supernova Remnants
Bartel, N., Shapiro, I. I., Jauncey, D. L., Kemball, A., Whitney, A. R., Rogers, A. E. E., Preston, R. A., & Jones, D. L. (1988). Radio observations of SN 1987A. In M. Kafatos, & A. G. Michalitsianos (Eds.), Supernova 1987A in the Large Magellanic Cloud: Proceedings of the Fourth George Mason Astrophysics Workshop (pp. 81-86). Cambridge University Press.