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dc.contributor.authorQiao, H.
dc.contributor.authorWalsh, Andrew
dc.contributor.authorShen, Z.
dc.contributor.authorDawson, J.
dc.date.accessioned2017-03-15T22:27:35Z
dc.date.available2017-03-15T22:27:35Z
dc.date.created2017-03-14T06:55:53Z
dc.date.issued2016
dc.identifier.citationQiao, H. and Walsh, A. and Shen, Z. and Dawson, J. 2016. Ground-state OH maser distributions in the Galactic Centre region, in Crocker, R. and Longmore, S. and Bicknell, G. (eds), Proceedings of the International Astronomical Union Symposia and Colloquia: The Multi-Messenger Astrophysics of the Galactic Centre, Jul 18-20 2016, 11 (S322), pp. 141-142. Palm Cove, Australia: IAU.
dc.identifier.urihttp://hdl.handle.net/20.500.11937/50688
dc.identifier.doi10.1017/S1743921316011765
dc.description.abstract

Ground-state OH masers identified in the Southern Parkes Large-Area Survey in Hydroxyl were observed with the Australia Telescope Compact Array to obtain positions with high accuracy (~1 arcsec). We classified these OH masers into evolved star OH maser sites, star formation OH maser sites, supernova remnant OH maser sites, planetary nebula OH maser sites and unknown maser sites using their accurate positions. Evolved star and star formation OH maser sites in the Galactic Centre region (between Galactic longitudes of -5° to +5° and Galactic latitudes of -2° and +2°) were studied in detail to understand their distributions.

dc.titleGround-state OH maser distributions in the Galactic Centre region
dc.typeConference Paper
dcterms.source.volume11
dcterms.source.startPage141
dcterms.source.endPage142
dcterms.source.issn1743-9213
dcterms.source.titleProceedings of the International Astronomical Union
dcterms.source.seriesProceedings of the International Astronomical Union
curtin.departmentCurtin Institute of Radio Astronomy (Physics)
curtin.accessStatusOpen access


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