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Cara Battersby edited section_The_Dense_ISM_Discussions__.tex
about 9 years ago
Commit id: d25f8372c16fa172731e01042d7654f0a6e934ff
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What do we still need to understand from the kinematics? Are positions every uniquely associated with a given kinematic signature? How can we describe the turbulence?
What explains the "cloud collision" kinematics often seen toward CMZ clouds \citep{Tanaka2015a,Tanaka2014a,Oka2012a}?
Comparison of H2CO and NH3 temperatures and morphology -- large and small scales