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Need to create a model for chemisputtering in molecular clouds, in line with the currently accepted theory. Also need to add in dust destruction via supernovae.
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1. Review a paper Sihan read
http://adsabs.harvard.edu/abs/2014MNRAS.439..936F
[Fujimoto+14: Do giant molecular clouds care about the galactic structure?]
2. Going through working progress SCUBA2…
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reported by: @CloudyLex
this paper gives attenuation as simple fit.
```
A&A 501, 619-631 (2009)
DOI: 10.1051/0004-6361/200911794
Cosmic-ray ionization of molecular clouds
M. Padovani1, 2, D. Galli…
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reported by: @CloudyLex
about 50% larger than our default
```
Title:
The cosmic ray ionization rate in the Galactic disk, as determined from observations of molecular ions
Authors:
Neufeld, David…
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reported by: @CloudyLex
```
Title:
The photodissociation and chemistry of CO isotopologues: applications to interstellar clouds and circumstellar disks
Authors:
Visser, R.; van Dishoeck, E. F.; B…
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reported by: @CloudyLex
we should look into this
```
Title:
Cosmic-ray and X-ray Heating of Interstellar Clouds and Protoplanetary Disks
Authors:
Glassgold, Alfred E.; Galli, Daniele; Padovani,…
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reported by: @CloudyLex
we now use rough guesses - this paper quantifies them
```
Goldsmith.P17Electron-Excitation-of-High-Dipole (article)
Electron Excitation of High Dipole Moment Molecules Re-ex…
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reported by: @CloudyLex
extensive discussion of HD chemistry and cooling in primordial collapse context. We need to update the H- rates and include HD.
http://arxiv.org/abs/1009.1087v1
Suppressi…
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**Is your feature request related to a problem? Please describe.**
A quick diagram of the topic is presented in the second post below.
Dear developers, I work in the field of molecular dynamics wh…
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We should restrict the scope to evaporating globules and knots. That is, excluding blister flows and champagne flows
So the main categories of ionized photoevaporation flows are:
1. In H II regi…