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dc.contributor.authorGalvin, T.
dc.contributor.authorFilipovic, M.
dc.contributor.authorTothill, N.
dc.contributor.authorCrawford, E.
dc.contributor.authorO Brien, A.
dc.contributor.authorSeymour, Nick
dc.contributor.authorPannuti, T.
dc.contributor.authorKosakowski, A.
dc.contributor.authorSharma, B.
dc.date.accessioned2017-01-30T14:50:34Z
dc.date.available2017-01-30T14:50:34Z
dc.date.created2016-01-18T20:00:50Z
dc.date.issued2014
dc.identifier.citationGalvin, T. and Filipovic, M. and Tothill, N. and Crawford, E. and O Brien, A. and Seymour, N. and Pannuti, T. et al. 2014. Radio-continuum study of the nearby sculptor group galaxies. Part 3: NGC 7793 at λ=12.2, 6 and 3 cm. Astrophysics and Space Science. 353 (2): pp. 603-611.
dc.identifier.urihttp://hdl.handle.net/20.500.11937/41326
dc.identifier.doi10.1007/s10509-014-2051-3
dc.description.abstract

We re-examine a series of archived centimetre radio-continuum observations (λ=16, 6 and 3 cm) focusing on NGC 7793 using the Australia Telescope Compact Array. These new images are both very sensitive (σ=0.011 mJy/beam) and feature reasonably high angular resolution (down to <3″). Using these images, a total of 76 discrete radio sources are identified, of which 57 have been classified. We also studied the radio component of the micro-quasar NGC7793-S26 which shows two distinct regions of somewhat steep spectral index (α) between −0.3 and −0.7.

dc.titleRadio-continuum study of the nearby sculptor group galaxies. Part 3: NGC 7793 at λ=12.2, 6 and 3 cm
dc.typeJournal Article
dcterms.source.volume353
dcterms.source.number2
dcterms.source.startPage603
dcterms.source.endPage611
dcterms.source.issn0004-640X
dcterms.source.titleAstrophysics and Space Science
curtin.departmentDepartment of Physics and Astronomy
curtin.accessStatusFulltext not available


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