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The Elliptical/Spiral Pair of Galaxies NGC 5090/5091

Published online by Cambridge University Press:  25 April 2016

R.M. Smith  and
G.V. Bicknell
R.M. Smith
Affiliation:
Mount Stromlo and Siding Spring Observatories, Australian National University
G.V. Bicknell
Affiliation:
Mount Stromlo and Siding Spring Observatories, Australian National University
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Extract

PKS 1318-43 was first identified with the elliptical galaxy NGC 5090 by Ekers (1969) in the Parkes catalogue. Schilizzi and McAdam (1975) mapped the source with 2.9 arcmin resolution at 408 MHz using the Mills Cross, resolving the source into an extended double structure approximately 15 arcmin in extent at p.a. 36°. Schilizzi (1975) also noted a possible optical link with an edge-on spiral (NGC 5091) ~75 arcsec to the south-east. Figure 1 shows a print of the two galaxies taken from the UK Schmidt J survey film. During 1980, in collaboration with K. J. Wellington, RMS mapped the source at 1415 MHz with the Fleurs Synthesis Telescope (FST, Christiansen 1973).

Type
Contributions
Information
Publications of the Astronomical Society of Australia , Volume 5 , Issue 2 , 1983 , pp. 251 - 254
Copyright
Copyright © Astronomical Society of Australia 1983

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References

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