Radio observations of SN 1987AThe 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.
Document ID
19890041490
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Bartel, N. (Harvard-Smithsonian Center for Astrophysics Cambridge, MA, United States)
Shapiro, I. I. (Harvard-Smithsonian Center for Astrophysics Cambridge, MA, United States)
Jauncey, D. L. (CSIRO Div. of Radiophysics, Epping, Australia)
Kemball, A. (Hartebeesthoek Radio Astronomy Observatory Johannesburg, Republic of South Africa, United States)
Whitney, A. R. (Harvard-Smithsonian Center for Astrophysics Cambridge, MA, United States)
Rogers, A. E. E. (Haystack Observatory Westford, MA, United States)
Preston, R. A. (Harvard-Smithsonian Center for Astrophysics Cambridge, MA, United States)
Jones, D. L. (California Institute of Technology Jet Propulsion Laboratory, Pasadena, United States)