Radio-continuum study of the nearby sculptor group galaxies. Part 3: NGC 7793 at λ=12.2, 6 and 3 cm

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 ima...

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Main Authors: Galvin, T., Filipovic, M., Tothill, N., Crawford, E., O Brien, A., Seymour, Nick, Pannuti, T., Kosakowski, A., Sharma, B.
Format: Journal Article
Published: 2014
Online Access:http://hdl.handle.net/20.500.11937/41326
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author Galvin, T.
Filipovic, M.
Tothill, N.
Crawford, E.
O Brien, A.
Seymour, Nick
Pannuti, T.
Kosakowski, A.
Sharma, B.
author_facet Galvin, T.
Filipovic, M.
Tothill, N.
Crawford, E.
O Brien, A.
Seymour, Nick
Pannuti, T.
Kosakowski, A.
Sharma, B.
author_sort Galvin, T.
building Curtin Institutional Repository
collection Online Access
description 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.
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institution Curtin University Malaysia
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publishDate 2014
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spelling curtin-20.500.11937-413262018-03-29T09:07:10Z Radio-continuum study of the nearby sculptor group galaxies. Part 3: NGC 7793 at λ=12.2, 6 and 3 cm Galvin, T. Filipovic, M. Tothill, N. Crawford, E. O Brien, A. Seymour, Nick Pannuti, T. Kosakowski, A. Sharma, B. 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. 2014 Journal Article http://hdl.handle.net/20.500.11937/41326 10.1007/s10509-014-2051-3 restricted
spellingShingle Galvin, T.
Filipovic, M.
Tothill, N.
Crawford, E.
O Brien, A.
Seymour, Nick
Pannuti, T.
Kosakowski, A.
Sharma, B.
Radio-continuum study of the nearby sculptor group galaxies. Part 3: NGC 7793 at λ=12.2, 6 and 3 cm
title Radio-continuum study of the nearby sculptor group galaxies. Part 3: NGC 7793 at λ=12.2, 6 and 3 cm
title_full Radio-continuum study of the nearby sculptor group galaxies. Part 3: NGC 7793 at λ=12.2, 6 and 3 cm
title_fullStr Radio-continuum study of the nearby sculptor group galaxies. Part 3: NGC 7793 at λ=12.2, 6 and 3 cm
title_full_unstemmed Radio-continuum study of the nearby sculptor group galaxies. Part 3: NGC 7793 at λ=12.2, 6 and 3 cm
title_short Radio-continuum study of the nearby sculptor group galaxies. Part 3: NGC 7793 at λ=12.2, 6 and 3 cm
title_sort radio-continuum study of the nearby sculptor group galaxies. part 3: ngc 7793 at λ=12.2, 6 and 3 cm
url http://hdl.handle.net/20.500.11937/41326