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dc.contributor.authorDawson, J.
dc.contributor.authorWalsh, Andrew
dc.date.accessioned2017-03-15T22:27:37Z
dc.date.available2017-03-15T22:27:37Z
dc.date.created2017-03-14T06:55:53Z
dc.date.issued2016
dc.identifier.citationDawson, J. and Walsh, A. 2016. OH as a Probe of The Milky Way's Hidden Gas: First Results from SPLASH, in Jablonka, P. and Andre, P. and van der Tak, F. (eds), Proceedings of the 315th International Astronomical Union Symposium: From Interstellar Clouds to Star-Forming Galaxies : Universal Processes?, Aug 3-7 2015, Honolulu, USA: IAU.
dc.identifier.urihttp://hdl.handle.net/20.500.11937/50703
dc.identifier.doi10.1017/S174392131600778X
dc.description.abstract

SPLASH (the Southern Parkes Large-Area Survey in Hydroxyl) is a deep survey of ground-state OH absorption and emission from the Galactic Plane, as well as an unbiased search for OH masers. Key early results include the detection of a rich and complex distribution of diffuse, optically thin OH with strongly non-thermal excitation temperatures, and the detection of numerous new maser sources. The survey aims to use OH as a probe of CO-dark H2 ISM Galactic scales, with future plans including comprehensive comparisons with CO and Hi, as well as non-LTE excitation modelling of the four ground-state lines.

dc.titleProbe of The Milky Way's Hidden Gas: First Results from SPLASH
dc.typeConference Paper
dcterms.source.volume315
dcterms.source.titleFrom interstellar clouds to star-forming galaxies: universal processes?
dcterms.source.seriesFROM INTERSTELLAR CLOUDS TO STAR-FORMING GALAXIES: UNIVERSAL PROCESSES?
dcterms.source.isbn978-1-107-13520-8
dcterms.source.conference315th Symposium of the International-Astronomical-Union
curtin.departmentCurtin Institute of Radio Astronomy (Physics)
curtin.accessStatusFulltext not available


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