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Absorption lines and the radio structure of quasars

Published online by Cambridge University Press:  19 July 2016

G. Swarup ,
D.J. Saikia ,
M. Beltrametti ,
R.P. Sinha  and
C.J. Salter
G. Swarup
Affiliation:
Tata Inst. of Fundamental Res., P. Box 1234, Bangalore, India
D.J. Saikia
Affiliation:
Tata Inst. of Fundamental Res., P. Box 1234, Bangalore, India
M. Beltrametti
Affiliation:
Max Planck Inst. Phys. Astrophys., Garching bei Munchen, FRG
R.P. Sinha
Affiliation:
Sys. and Applied Sc. Corpn. Hyattesville, Md 20784, U.S.A.
C.J. Salter
Affiliation:
Nat. Radio Astr. Obs., Tuscon, Arizona 85721, U.S.A.

Abstract

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We have investigated a possible relationship between the radio structure of quasars and their absorption line systems with velocities, V, in the range 3000–18000 km s−1 and find a marginal trend for such quasars to have compact radio structures (Swarup et al. 1986).

Type
II. Continuum Emission
Information
Symposium - International Astronomical Union , Volume 119: Quasars , 1986 , pp. 195 - 196
Copyright
Copyright © Reidel 1986 

References

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