1983
DOI: 10.1017/s132335800001701x
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Maps of Centaurus A from Molonglo and Culgoora

Abstract: While Centaurus A (NGC 5128) is not a particularly powerful radio galaxy, its proximity (˜ 5 Mpc) permits us to obtain linear resolution an order of magnitude better than can be obtained for the more powerful, distant radio galaxies. Thus one can hope to make meaningful comparisons between the morphologies seen over the electromagnetic spectrum from γ-rays to metre waves. This should lead to a more complete understanding of the energy production mechanisms and evolutionary histories of these objects.

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Cited by 6 publications
(3 citation statements)
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“…Bending and buoyancy effects (e.g. 119,235,283) may also be present and--unless the jet is denser than the ambient medium--lateral motions may excite surface instabilities, whose growth also alters the shape of the jet (12). Linear instability theory may be inadequate to describe any mode that grows sufficiently to become detectable on radio maps.…”
Section: Jet Wigglingmentioning
confidence: 99%
“…Bending and buoyancy effects (e.g. 119,235,283) may also be present and--unless the jet is denser than the ambient medium--lateral motions may excite surface instabilities, whose growth also alters the shape of the jet (12). Linear instability theory may be inadequate to describe any mode that grows sufficiently to become detectable on radio maps.…”
Section: Jet Wigglingmentioning
confidence: 99%
“…Although a VLA map published in 1981 offered more fine detail in the central region, the Australian observations provided flux densities and spectral data for the two inner lobes of this galaxy. Finally, Slee, Sheridan, Dulk and Little (1983) concluded by discussing possible mechanisms that could explain the galaxy's radio and X-ray emission.…”
Section: Figure 50mentioning
confidence: 99%
“…(2.15) using data from [54] and [55][56][57][58] respectively. This yields enhancement factors of the form…”
mentioning
confidence: 99%