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Two-Sided Radio Jets in B1524–136

Published online by Cambridge University Press:  05 March 2013

F. Mantovani ,
M. Bondi ,
D. J. Saikia ,
W. Junor ,
C. J. Salter  and
R. Ricci
F. Mantovani
Affiliation:
Istituto di Radioastronomia, Via P. Gobetti, 101, 40129 Bologna, Italy. fmantovani@ira.cnr.it, bondi@ira.cnr.it
M. Bondi
Affiliation:
Istituto di Radioastronomia, Via P. Gobetti, 101, 40129 Bologna, Italy. fmantovani@ira.cnr.it, bondi@ira.cnr.it
D. J. Saikia
Affiliation:
Department of Physics and Astronomy, University of New Mexico, Albuquerque, NM 87131. bjunor@as.unm.edu
W. Junor
Affiliation:
Department of Physics and Astronomy, University of New Mexico, Albuquerque, NM 87131. bjunor@as.unm.edu
C. J. Salter
Affiliation:
SISSA, Via Beirut 4, 34014 Trieste, Italy.ricci@sissa.it
R. Ricci
Affiliation:
SISSA, Via Beirut 4, 34014 Trieste, Italy.ricci@sissa.it
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Abstract

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We present global VLBI and VLBA observations of the compact steep spectrum quasar B1524–136. These observations reveal well-defined radio jets on both sides of the active nucleus. Also, the overall radio structure appears highly distorted and asymmetric with the counter-jet exhibiting several oscillations. A possible scenario is one in which jet and counter-jet are inclined at about 25° and 75° to the line of sight respectively and an environment which is dense on the jet side. Possible implications of these results are discussed.

Keywords

galaxies: activegalaxies: jetsgalaxies: nucleiquasars: generalquasars: individual (B1524–136)radio continuum: galaxies
Type
GPS/CSS Workshop
Information
Publications of the Astronomical Society of Australia , Volume 20 , Issue 1 , 2003 , pp. 85 - 87
Copyright
Copyright © Astronomical Society of Australia 2003

References

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