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A study of one-sided radio quasars

Published online by Cambridge University Press:  19 July 2016

D.J. Saikia ,
P. Shastri ,
T.J. Cornwell  and
C.J. Salter
D.J. Saikia
Affiliation:
Tata Institute of Fundamental Research, Bangalore, India
P. Shastri
Affiliation:
Tata Institute of Fundamental Research, Bangalore, India
T.J. Cornwell
Affiliation:
NRAO, Socorro, New Mexico, U.S.A.
C.J. Salter
Affiliation:
IRAM, Granada, Spain

Extract

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Although most powerful extended radio quasars have lobes of radio emission on opposite sides of the nuclear component, a significant number appear to have extended emission on only one side. We have observed ∼40 such sources (mostly from the compilation of Kapahi 1981) with the VLA, to confirm their classification and study their properties.

Type
II. Continuum Emission
Information
Symposium - International Astronomical Union , Volume 119: Quasars , 1986 , pp. 219 - 220
Copyright
Copyright © Reidel 1986 

References

Kapahi, V.K., 1981. J. Astrophys. Astr. 2, 43.Google Scholar
Perley, R.A., 1982. Astr. J. 87, 859.Google Scholar
Saikia, D.J., Shastri, P., 1984. Mon. Not. R. astr. Soc. 211, 47.CrossRefGoogle Scholar
Rudnick, L., Edgar, B.K., 1984. Astrophys. J. 279, 74.Google Scholar