Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
University of Tasmania
U Tasmania
Uni of Tas
Univ. of Tasmania
School of Mathematics and Physics, University of Tasmania
School of Mathematics and Physics, University of Tasmania, Private Bag 37, Hobart, TAS 7001, Australia
Department of Physics, University of Tasmania, G.P.O. Box 252C, Hobart, Tasmania 7001, Australia
Physics Department, University of Tasmania, GPO Box 252c, Hobart, Tas 7001, Australia
Department of Physics, University of Tasmania, GPO Box 252-21, Hobart, TAS 7001, Australia
Physics Department, University of Tasmania, GPO Box 252c, Hobart, Tasmania 7001, Australia
School of Mathematics and Physics, University of Tasmania, Private Bag 37, Hobart, Tasmania 7001, Australia
School of Mathematics and Physics, University of Tasmania, Private Bag 21, Hobart, Tasmania 7001, Australia
School of Mathematics and Physics, University of Tasmania, Private Bag 21, Hobart 7001, TAS, Australia
UTas
School of Mathematics and Physics, University of Tasmania, Hobart, Tasmania, Australia
University of Tasmania, Hobart, Australia
School of Mathematics and Physics, University of Tasmania, GPO Box 252-21, Hobart, Tasmania 7001, Australia of Physics, University of Tasmania, G.P.O. Box 252C, Hobart, Tasmania 7001, Australia of Mathematics and Physics, University of Tasmania, Australia
School of Mathematics and Physics, University of Tasmania, Private Bag 37, Hobart, Tasmania 7001, Australia.
School of Mathematics and Physics, Private Bag 37, University of Tasmania, Hobart, Tasmania 7001, Australia
School of Mathematics and Physics, University of Tasmania, Private Bag 37
12.2-GHz methanol masers associated with 1.2-mm dust clumps: Quantifying high-mass star formation evolutionary schemes
37 GHz methanol masers : Horsemen of the Apocalypse for the class II methanol maser phase?
6.7GHz methanol masers survey of low-mass YSO (Minier+, 2003)
95GHz methanol maser survey toward GLIMPSE EGOs (Chen+, 2011)
A 95 GHz Class I Methanol Maser Survey Toward A Sample of GLIMPSE Point Sources Associated with BGPS Clumps
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