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Trial run for importing the nublado.org Trac tickets as GitHub issues
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electron - molecule collisions (trac #401) #403

Open cloudy-bot opened 7 years ago

cloudy-bot commented 7 years ago

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-examined 
Goldsmith, P. F. & Kauffmann, J.
2017, \apj, 841, 25

ABSTRACT: Emission from high-dipole moment molecules such as HCN allows determination of the density 
in molecular clouds, and is often considered to trace the dense'' gas available for star formation. We assess 
the importance of electron excitation in various environments. The ratio of the rate coefficients for 
electrons and H2 molecules, ~=105 for HCN, yields the requirements for electron excitation to be of 
practical importance if n(
```H```2)<=slant {10}5.5 {{cm}}-3 and X(```e```-)>=slant {10}-5, where the 
numerical factors reflect the critical values {n}{{c}}(```H```2) and {X}* (```e```-). This indicates that in 
regions where a large fraction of carbon is ionized, X(```e```-) will be large enough to make electron 
excitation significant. The situation is in general similar for other high-density tracers,'' including HCO+, CN, 
and CS. But there are significant differences in the critical electron fractional abundance, {X}* (```e```-), 
defined by the value required for equal effect from collisions with H2 and e-. Electron excitation is, for 
example, unimportant for CO and C+. Electron excitation may be responsible for the surprisingly large 
spatial extent of emission from dense gas tracers in some molecular clouds. The enhanced estimates for 
HCN abundances and HCN/CO and HCN/HCO+ ratios observed in the nuclear regions of luminous galaxies 
may be in part a result of electron excitation of high dipole moment tracers. The importance of electron 
excitation will depend on detailed models of the chemistry, which may well be non-steady state and non-
static.

KEYWORDS: ISM: molecules, molecular processes, photon-dominated region: PDR
NOTE: 

LOCAL FILE : ~/Dropbox/literature/molecules/collisions/electronCollisions/Goldsmith.P17Electron-Excitation-of-High-Dipole.pdf
REMOTE URL : http://dx.doi.org/10.3847/1538-4357/aa6f12
ADS URL : http://adsabs.harvard.edu/abs/2017ApJ...841...25G

Migrated from https://www.nublado.org/ticket/401

{
    "status": "new",
    "changetime": "2019-02-04T13:07:06Z",
    "_ts": "1549285626580696",
    "description": "we now use rough guesses - this paper quantifies them\n{{{\nGoldsmith.P17Electron-Excitation-of-High-Dipole (article)\nElectron Excitation of High Dipole Moment Molecules Re-examined \nGoldsmith, P. F. & Kauffmann, J.\n2017, \\apj, 841, 25\n\nABSTRACT: Emission from high-dipole moment molecules such as HCN allows determination of the density \nin molecular clouds, and is often considered to trace the dense'' gas available for star formation. We assess \nthe importance of electron excitation in various environments. The ratio of the rate coefficients for \nelectrons and H2 molecules, ~=105 for HCN, yields the requirements for electron excitation to be of \npractical importance if n({{{H}}}2)<=slant {10}5.5 {{cm}}-3 and X({{{e}}}-)>=slant {10}-5, where the \nnumerical factors reflect the critical values {n}{{c}}({{{H}}}2) and {X}* ({{{e}}}-). This indicates that in \nregions where a large fraction of carbon is ionized, X({{{e}}}-) will be large enough to make electron \nexcitation significant. The situation is in general similar for other high-density tracers,'' including HCO+, CN, \nand CS. But there are significant differences in the critical electron fractional abundance, {X}* ({{{e}}}-), \ndefined by the value required for equal effect from collisions with H2 and e-. Electron excitation is, for \nexample, unimportant for CO and C+. Electron excitation may be responsible for the surprisingly large \nspatial extent of emission from dense gas tracers in some molecular clouds. The enhanced estimates for \nHCN abundances and HCN/CO and HCN/HCO+ ratios observed in the nuclear regions of luminous galaxies \nmay be in part a result of electron excitation of high dipole moment tracers. The importance of electron \nexcitation will depend on detailed models of the chemistry, which may well be non-steady state and non-\nstatic.\n\nKEYWORDS: ISM: molecules, molecular processes, photon-dominated region: PDR\nNOTE: \n\nLOCAL FILE : ~/Dropbox/literature/molecules/collisions/electronCollisions/Goldsmith.P17Electron-Excitation-of-High-Dipole.pdf\nREMOTE URL : http://dx.doi.org/10.3847/1538-4357/aa6f12\nADS URL : http://adsabs.harvard.edu/abs/2017ApJ...841...25G\n\n}}}",
    "reporter": "gary",
    "cc": "",
    "resolution": "",
    "time": "2017-09-11T20:50:32Z",
    "component": "atomic/molecular data base",
    "summary": "electron - molecule collisions",
    "priority": "major",
    "keywords": "",
    "version": "",
    "milestone": "no milestone",
    "owner": "nobody",
    "type": "enhancement"
}
cloudy-bot commented 7 years ago

@peter-van-hoof-noaccount changed milestone from "" to "no milestone"