VLBI structure of the QSO 3C286

Kus, A. J.; Marecki, A.; Neff, S.; Van Ardenne, A.; Wilkinson, P. N.

Observations 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

Meeting Information

IAU Symposium on the Impace of VLBI on Astrophysics and Geophysics(Cambridge, MA)

Distribution Limits

Public

Other

NTRS

NTRS - NASA Technical Reports Server