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Probing the Accretion Region of NGC 1275 with VLBI

Published online by Cambridge University Press:  12 April 2016

R.C. Walker ,
K.I. Kellermann ,
V. Dhawan ,
J. D. Romney ,
J. M. Benson ,
R. C. Vermeulen  and
W. Alef
R.C. Walker
Affiliation:
National Radio Astronomy Observatory, Socorro, NM, U.S.A.
K.I. Kellermann
Affiliation:
National Radio Astronomy Observatory, Charlottesville, VA, U.S.A.
V. Dhawan
Affiliation:
National Radio Astronomy Observatory, Socorro, NM, U.S.A.
J. D. Romney
Affiliation:
National Radio Astronomy Observatory, Socorro, NM, U.S.A.
J. M. Benson
Affiliation:
National Radio Astronomy Observatory, Socorro, NM, U.S.A.
R. C. Vermeulen
Affiliation:
Netherlands Foundation for Radio Astronomy, Dwingeloo, The Netherlands
W. Alef
Affiliation:
Max-Planck-Institut für Radioastronomie, Bonn, Germany

Abstract

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Multi-frequency VLBA observations were used to study the magnitude and radial dependence of free-free absorption of the radio emission from the counterjet in 3C 84.

Type
Research Article
Information
International Astronomical Union Colloquium , Volume 164: Radio Emission from Galactic and Extragalactic Compact Sources , 1998 , pp. 133 - 134
Copyright
Copyright © Astronomical Society of the Pacific 1998

References

Walker, R.C., Romney, J.D., & Benson, J.M. 1994. ApJ, 430, L45–48.CrossRefGoogle Scholar
Vermeulen, R.C., Readhead, A.C.S., & Backer, D.C. 1994. ApJ, 430, L41–44.CrossRefGoogle Scholar
Levinson, A., Laor, A., & Vermeulen, R.C. 1995. ApJ, 448, 589–599.Google Scholar