this is for holding javascript data
Adam Ginsburg added section_The_Dense_ISM_Discussions__.tex
about 9 years ago
Commit id: 1f61891870fd7f8045f5ea0d31d4235fd8222c29
deletions | additions
diff --git a/section_The_Dense_ISM_Discussions__.tex b/section_The_Dense_ISM_Discussions__.tex
new file mode 100644
index 0000000..8a7f47e
--- /dev/null
+++ b/section_The_Dense_ISM_Discussions__.tex
...
\section{The "Dense" ISM}
Discussions on what would normally be considered high-density gas ($n\sim10^4$ cm$^{-3}$) but in the CMZ is "typical".
What are the true gas densities and what is the density distribution? Which clouds are bound? Are they supported by turbulence, magnetic fields, thermal pressure, shear, or are they freely collapsing?
What are the magnetic fields and temperatures of these clouds?
What is the geometry of the molecular gas in the CMZ - is there really a ring? Are the clouds on elliptical orbits? Which orbits?
