Towards a three-dimensional distribution of the molecular clouds in the Galactic Centre

Towards a three-dimensional distribution of the molecular clouds in the Galactic Centre

We present a study of the three-dimensional structure of the molecular clouds in the Galactic Centre (GC) using CO emission and OH absorption lines. Two CO isotopologue lines, $^{12}$CO ($J$=1$\rightarrow$0) and $^{13}$CO ($J$=1$\rightarrow$0), and four OH ground-state transitions, surveyed by the S...

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Bibliographic Details
Main Authors: Yan, Q., Walsh, A., Dawson, J., Macquart, Jean-Pierre, Blackwell, R., Burton, M., Rowell, G., Zhang, B., Xu, Y., Tang, Z., Hancock, Paul
Format: Journal Article
Published: Oxford University Press 2017
Online Access:http://hdl.handle.net/20.500.11937/57869
http://dx.doi.org/10.1093/mnras/stx1724

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