Ticket #173 (new enhancement)
HD chemistry, cooling
|Reported by:||gary||Owned by:|
|Priority:||good to do||Milestone:|
|Component:||atomic/molecular data base||Version:||trunk|
extensive discussion of HD chemistry and cooling in primordial collapse context. We need to update the H- rates and include HD.
Suppression of HD–cooling in protogalactic gas clouds by Lyman-Werner radiation J. Wolcott-Green1? and Z. Haiman 2?