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Radio Continuum Emission from Sculptor Galaxies

Published online by Cambridge University Press:  25 April 2016

J . I. Harnet
J . I. Harnet*
Affiliation:
School of Physics, University of Sydney
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Abstract

The five major members of the Sculptor Group of galaxies and NGC 45 have been observed with the Molonglo observatory synthesis telescope. NGC 247 and NGC 300 were not detected and upper limits to their 843 MHz flux densities are given. Radio emission from NGC 7793 is discussed with particular attention to its morphology, radial dependence compared with that of the blue light and possible coincidences between HII regions and 843 MHz peak flux densities.

Type
Contributions
Information
Publications of the Astronomical Society of Australia , Volume 6 , Issue 3 , 1986 , pp. 325 - 329
Copyright
Copyright © Astronomical Society of Australia 1986

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