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1.2 mm emission from Cen A

Published online by Cambridge University Press:  26 May 2016

Zita Banhidi ,
Rolf Chini  and
Marcus Albrecht
Zita Banhidi
Affiliation:
Astronomisches Institut Ruhr-Universität Bochum, D-44780 Bochum, Universitätsstraße 150, Germany
Rolf Chini
Affiliation:
Astronomisches Institut Ruhr-Universität Bochum, D-44780 Bochum, Universitätsstraße 150, Germany
Marcus Albrecht
Affiliation:
Astronomisches Institut Ruhr-Universität Bochum, D-44780 Bochum, Universitätsstraße 150, Germany

Abstract

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Centaurus A is the closest active radio galaxy at a distance of around 3.5 Mpc. New 1.2 mm imaging performed with SIMBA at the Swedish ESO Submillimetre Telescope (SEST) in Chile gives an insight into the distribution of thermal and non-thermal emission. Apart from extended synchrotron emission in the radio lobes we have detected the unresolved AGN core and the characteristic dust lane.

Type
Part 5: Clusters and Ellipticals
Information
Symposium - International Astronomical Union , Volume 220: Dark Matter in Galaxies , 2004 , pp. 183 - 184
Copyright
Copyright © Astronomical Society of the Pacific 2004 

References

Burns, J. O., Feigelson, E. D. & Schreier, E. J. 1983, ApJ, 273, 128.Google Scholar
Clarke, D. A., Burns, J. O. & Norman, M. L. 1992, ApJ, 395, 444.Google Scholar
Condon, J. J., Helou, G., Sanders, D. B. & Soifer, B. T. 1996, ApJS, 103, 81.Google Scholar
Nyman, L.-Å., Lerner, M., Nielbock, M., et al. 2001, ESO Messenger, 106, 40.Google Scholar