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dc.contributor.authorEdwards, P.
dc.contributor.authorOjha, R.
dc.contributor.authorDodson, R.
dc.contributor.authorLovell, J.
dc.contributor.authorReynolds, J.
dc.contributor.authorTzioumis, A.
dc.contributor.authorQuick, J.
dc.contributor.authorNicolson, G.
dc.contributor.authorTingay, Steven
dc.date.accessioned2018-05-18T07:57:28Z
dc.date.available2018-05-18T07:57:28Z
dc.date.created2018-05-18T00:23:29Z
dc.date.issued2018
dc.identifier.citationEdwards, P. and Ojha, R. and Dodson, R. and Lovell, J. and Reynolds, J. and Tzioumis, A. and Quick, J. et al. 2018. VLBI Observations of Southern Gamma-Ray Sources. III. Publications of the Astronomical Society of Australia. 35: Article ID e009.
dc.identifier.urihttp://hdl.handle.net/20.500.11937/67158
dc.identifier.doi10.1017/pasa.2018.4
dc.description.abstract

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.

dc.publisherCambridge University Press
dc.titleVLBI Observations of Southern Gamma-Ray Sources. III
dc.typeJournal Article
dcterms.source.issn1323-3580
dcterms.source.titlePublications of the Astronomical Society of Australia
curtin.departmentCurtin Institute of Radio Astronomy (Physics)
curtin.accessStatusOpen access


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