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VLBI structure of the QSO 3C286Observations of the quasar 3C286 with the EVN at 609 and 1420 MHz are reported. Results are presented on source size, the steepening of the spectral index, the IC X-ray flux, and surface brightness temperature. It is concluded that 3C286 appears to be not as energetic as the other 3C sources of the class.
Document ID
19890026366
Document Type
Conference Paper
Authors
Kus, A. J. (NASA Goddard Space Flight Center Greenbelt, MD, United States)
Marecki, A. (Torun Radio Astronomy Observatory Poland)
Neff, S. (NASA Goddard Space Flight Center Greenbelt, MD, United States)
Van Ardenne, A. (Dwingeloo Radiosterrenwacht, Netherlands)
Wilkinson, P. N. (Manchester, Victoria University Jodrell Bank, United Kingdom)
Date Acquired
August 14, 2013
Publication Date
January 1, 1988
Subject Category
ASTROPHYSICS
Meeting Information
IAU Symposium on the Impace of VLBI on Astrophysics and Geophysics(Cambridge, MA)
Distribution Limits
Public
Copyright
Other