Publisher： Cambridge University Press
E-ISSN： 1743-9221|11|S322|85-89
ISSN： 1743-9213
Source： Proceedings of the International Astronomical Union, Vol.11, Iss.S322, 2017-02, pp. : 85-89
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Abstract
The central molecular zone (CMZ) hosts some of the most massive and dense molecular clouds and star clusters in the Galaxy, offering an important window into star formation under extreme conditions. Star formation in this extreme environment may be closely linked to the 3-D distribution and orbital dynamics of the gas. Here I discuss how our new, accurate description of the {
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