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Unusual Radio Structures in Markarian 6

Published online by Cambridge University Press:  25 May 2016

M.J. Kukula ,
A. Pedlar ,
S.A. Baum  and
A.J. Holloway
M.J. Kukula
Affiliation:
1 Institute for Astronomy - University of Edinburgh, Royal Observatory, Edinburgh EH9 3HJ, U.K.
A. Pedlar
Affiliation:
2 NRAL - University of Manchester, Jodrell Bank, Macclesfield SK11 9DL, U.K.
S.A. Baum
Affiliation:
3 STScI - 3700 San Martin Drive, Baltimore, U.S.A.
A.J. Holloway
Affiliation:
4 Department of Physics & Astronomy University of Manchester, Manchester, U.K.

Extract

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Markarian 6, a Seyfert Galaxy of type 1.5, is one of several Seyfert nuclei to be observed with MERLIN at 6 and 18 cm as part of a project to investigate the radio structures of these objects on sub–arcsecond scales (corresponding to scales of a few tens of parsecs at typical distances). The angular resolution of MERLIN at 6 cm is equivalent to that of the HST, making the radio images ideal for comparison with HST images of the optical Narrow–Line Region (NLR). In this paper we briefly discuss the results of our MERLIN observations of Markarian 6, along with a 6–cm Westerbork Synthesis Radio Telescope (WSRT) map of the arcsecond (kpc) scale radio emission. The data is discussed in more detail by Kukula et al. (1996) and Baum et al. (1993).

Type
Properties of Radio Sources
Information
Symposium - International Astronomical Union , Volume 175: Extragalactic Radio Sources , 1996 , pp. 177 - 178
Copyright
Copyright © Kluwer 1996 

References

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