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Centaurus A, the core of the problemThe bright, peculiar elliptical galaxy Centaurus A (NGC 5128, PKS 1322-427) was one of the first extragalactic radio sources to be optically identified (Bolton et al. 1949). At a distance of 4 Mpc, Centaurus A is the closest active radio galaxy and affords the highest linear imaging resolution (1 mas approximately equal to 0.02 pc) and hence the best prospects for studying an active nucleus close to the central radio source. We present the results of multi-epoch, 8.4-GHz, very long baseline interferometry (VLBI), imaging observations of the nucleus made over the past three years. The nucleus possesses a core-jet structure where the inner portion of the jet shows apparent linear motion with a velocity substantially less than the speed of light.
Document ID
19950052447
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Tingay, S. J.
(Australian National University Private Bag, Australia)
Jauncey, D. L.
(CSIRO Australia)
Preston, R. A.
(Jet Propulsion Laboratory, Pasadena, CA US, United States)
Reynolds, J. E.
(CSIRO Australia)
Meier, D. L.
(Jet Propulsion Laboratory, Pasadena, CA US, United States)
Tzioumis, A. K.
(CSIRO Australia)
Jones, D. L.
(Jet Propulsion Laboratory, Pasadena, CA US, United States)
King, E. A.
(University of Tasmania Australia)
Amy, S. W.
(University of Sydney Australia)
Biggs, J. D.
(Curtin University Australia)
Date Acquired
August 16, 2013
Publication Date
January 1, 1994
Publication Information
Publication: Australian Journal of Physics
Volume: 47
Issue: 5
ISSN: 0004-9506
Subject Category
Astronomy
Report/Patent Number
ISSN: 0004-9506
Accession Number
95A84046
Distribution Limits
Public
Copyright
Other

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