VLBI Observations of Southern Gamma-Ray Sources. III

We report the results of Long Baseline Array observations made in 2001 of ten southern sources proposed by Mattox et al. as counterparts to EGRET > 100 MeV gamma-ray sources. Source structures are compared with published data where available and possible superluminal motions identified in se...

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Main Authors: Edwards, P., Ojha, R., Dodson, R., Lovell, J., Reynolds, J., Tzioumis, A., Quick, J., Nicolson, G., Tingay, Steven
Format: Journal Article
Published: Cambridge University Press 2018
Online Access:http://hdl.handle.net/20.500.11937/67158
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author Edwards, P.
Ojha, R.
Dodson, R.
Lovell, J.
Reynolds, J.
Tzioumis, A.
Quick, J.
Nicolson, G.
Tingay, Steven
author_facet Edwards, P.
Ojha, R.
Dodson, R.
Lovell, J.
Reynolds, J.
Tzioumis, A.
Quick, J.
Nicolson, G.
Tingay, Steven
author_sort Edwards, P.
building Curtin Institutional Repository
collection Online Access
description We report the results of Long Baseline Array observations made in 2001 of ten southern sources proposed by Mattox et al. as counterparts to EGRET > 100 MeV gamma-ray sources. Source structures are compared with published data where available and possible superluminal motions identified in several cases. The associations are examined in the light of Fermi observations, indicating that the confirmed counterparts tend to have radio properties consistent with other identifications, including flat radio spectral index, high brightness temperature, greater radio variability, and higher core dominance.
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institution Curtin University Malaysia
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last_indexed 2025-11-14T10:32:31Z
publishDate 2018
publisher Cambridge University Press
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spelling curtin-20.500.11937-671582019-02-25T23:55:54Z VLBI Observations of Southern Gamma-Ray Sources. III Edwards, P. Ojha, R. Dodson, R. Lovell, J. Reynolds, J. Tzioumis, A. Quick, J. Nicolson, G. Tingay, Steven We report the results of Long Baseline Array observations made in 2001 of ten southern sources proposed by Mattox et al. as counterparts to EGRET > 100 MeV gamma-ray sources. Source structures are compared with published data where available and possible superluminal motions identified in several cases. The associations are examined in the light of Fermi observations, indicating that the confirmed counterparts tend to have radio properties consistent with other identifications, including flat radio spectral index, high brightness temperature, greater radio variability, and higher core dominance. 2018 Journal Article http://hdl.handle.net/20.500.11937/67158 10.1017/pasa.2018.4 Cambridge University Press fulltext
spellingShingle Edwards, P.
Ojha, R.
Dodson, R.
Lovell, J.
Reynolds, J.
Tzioumis, A.
Quick, J.
Nicolson, G.
Tingay, Steven
VLBI Observations of Southern Gamma-Ray Sources. III
title VLBI Observations of Southern Gamma-Ray Sources. III
title_full VLBI Observations of Southern Gamma-Ray Sources. III
title_fullStr VLBI Observations of Southern Gamma-Ray Sources. III
title_full_unstemmed VLBI Observations of Southern Gamma-Ray Sources. III
title_short VLBI Observations of Southern Gamma-Ray Sources. III
title_sort vlbi observations of southern gamma-ray sources. iii
url http://hdl.handle.net/20.500.11937/67158