this is for holding javascript data
Adam Ginsburg edited section_SMA_CMZ_8_GHz__.tex
about 9 years ago
Commit id: 48d05b04d58460a2d887a1fe68d461da7d5eefa4
deletions | additions
diff --git a/section_SMA_CMZ_8_GHz__.tex b/section_SMA_CMZ_8_GHz__.tex
index 96654ca..3482220 100644
--- a/section_SMA_CMZ_8_GHz__.tex
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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. Steve: free-fall times come from single-dish, large scale. Diederik: position along ridge dominates spread in density.
Lines mapped: H$_2$CO, C$^{18}$O, CH$_3$OH, $^{13}$CO, SiO.