deletions | additions       diff --git a/section_SMA_CMZ_8_GHz__.tex b/section_SMA_CMZ_8_GHz__.tex  index 2e6e0b9..bf62438 100644  --- a/section_SMA_CMZ_8_GHz__.tex  +++ b/section_SMA_CMZ_8_GHz__.tex 
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Data to become public when they are reduced.  How can we identify star forming cores? Original idea: hot core tracers + outflows. Does that work?