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VLBI Structure of the QSO 3C286

Published online by Cambridge University Press:  03 August 2017

A. J. Kus
Affiliation:
TRAO, Torun, Poland
A. Marecki
Affiliation:
TRAO, Torun, Poland
S. Neff
Affiliation:
NASA/GSFC, Washington, DC, USA
A. van Ardenne
Affiliation:
Radiosterrenwacht, Dwingeloo, Netherlands
P. N. Wilkinson
Affiliation:
NRAL, Jodrell Bank, United Kingdom

Extract

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The steep, small angular size QSO 3C286 (z = 0.846, mv = 17m) (Burbidge and Burbidge 1969) is a bright object in the radio band, which has a steep spectrum (α = −0.65, Sfα) from 1 GHz, peak in spectrum at about 100 MHz, and self-absorption below 50 MHz. 3C286 is a member of a well established class of radio sources (the CSSQSO) and is similar to 3C147, 3C309.1, and 3C380 in general.

Type
Extragalactic
Copyright
Copyright © Reidel 1988 

References

Burbidge, G. R., and Burbidge, E. M. 1969, Nature, 222, 735.CrossRefGoogle Scholar
Pearson, T. J., et al. 1980, Ap. J., 236, 714.CrossRefGoogle Scholar
Readhead, A. C. S., and Hewish, A. 1974, M. N. R. A. S., 78, 1.Google Scholar
Simon, R. S., et al. 1980, Ap. J., 236, 707.Google Scholar
van Breugel, W. J. M., et al. 1984, A. J., 89, 5.Google Scholar
Wilkinson, P.N., et al. 1979, Ap. J., 232, 365.Google Scholar