deletions | additions       diff --git a/section_SMA_CMZ_8_GHz__.tex b/section_SMA_CMZ_8_GHz__.tex  index 815fd47..588a7b0 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? CH$_3$OH masers, but incomplete/maybe just shock tracers? Evolutionary sequence in massive cores seen in dust ridge clouds.