update O III to new storey / badnell paper (trac #293)

reported by: @CloudyLex

Title:  
Collision strengths for nebular [O III] optical and infrared lines
Authors:    
Storey, P. J.; Sochi, Taha; Badnell, N. R.
Affiliation:    
AA(Department of Physics and Astronomy, University College London, Gower Street, London WC1E 6BT, UKt.sochi@ucl.ac.uk), AB(Department of Physics and Astronomy, University College London, Gower Street, London WC1E 6BT, UK), AC(Department of Physics, University of Strathclyde, Glasgow G4 0NG, UK)
Publication:    
Monthly Notices of the Royal Astronomical Society, Volume 441, Issue 4, p.3028-3039 (MNRAS Homepage)
Publication Date:   
07/2014
Origin: 
OUP
Astronomy Keywords: 
atomic data, atomic processes, radiation mechanisms: non-thermal, planetary nebulae: general, infrared: general
Abstract Copyright: 
2014 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society
DOI:    
10.1093/mnras/stu777
Bibliographic Code: 
2014MNRAS.441.3028S
Abstract

We present electron collision strengths and their thermally averaged values for the 
nebular forbidden lines of the astronomically abundant doubly ionized oxygen ion, 
O2+, in an intermediate coupling scheme using the Breit-Pauli relativistic terms as 
implemented in an R-matrix atomic scattering code. We use several atomic targets 
for the R-matrix scattering calculations including one with 72 atomic terms. We 
also compare with new results obtained using the intermediate coupling frame 
transformation method. We find spectroscopically significant differences against a 
recent Breit-Pauli calculation for the excitation of the [O III] ?4363 transition but 
confirm the results of earlier calculations.

Migrated from https://www.nublado.org/ticket/293

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    "status": "new",
    "changetime": "2019-02-04T13:07:06Z",
    "_ts": "1549285626580696",
    "description": "{{{\nTitle:\t\nCollision strengths for nebular [O III] optical and infrared lines\nAuthors:\t\nStorey, P. J.; Sochi, Taha; Badnell, N. R.\nAffiliation:\t\nAA(Department of Physics and Astronomy, University College London, Gower Street, London WC1E 6BT, UKt.sochi@ucl.ac.uk), AB(Department of Physics and Astronomy, University College London, Gower Street, London WC1E 6BT, UK), AC(Department of Physics, University of Strathclyde, Glasgow G4 0NG, UK)\nPublication:\t\nMonthly Notices of the Royal Astronomical Society, Volume 441, Issue 4, p.3028-3039 (MNRAS Homepage)\nPublication Date:\t\n07/2014\nOrigin:\t\nOUP\nAstronomy Keywords:\t\natomic data, atomic processes, radiation mechanisms: non-thermal, planetary nebulae: general, infrared: general\nAbstract Copyright:\t\n2014 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society\nDOI:\t\n10.1093/mnras/stu777\nBibliographic Code:\t\n2014MNRAS.441.3028S\nAbstract\n\nWe present electron collision strengths and their thermally averaged values for the \nnebular forbidden lines of the astronomically abundant doubly ionized oxygen ion, \nO2+, in an intermediate coupling scheme using the Breit-Pauli relativistic terms as \nimplemented in an R-matrix atomic scattering code. We use several atomic targets \nfor the R-matrix scattering calculations including one with 72 atomic terms. We \nalso compare with new results obtained using the intermediate coupling frame \ntransformation method. We find spectroscopically significant differences against a \nrecent Breit-Pauli calculation for the excitation of the [O III] ?4363 transition but \nconfirm the results of earlier calculations.\n}}}",
    "reporter": "gary",
    "cc": "",
    "resolution": "",
    "time": "2014-08-17T06:57:33Z",
    "component": "atomic/molecular data base",
    "summary": "update O III to new storey / badnell paper",
    "priority": "good to do",
    "keywords": "",
    "version": "trunk",
    "milestone": "no milestone",
    "owner": "nobody",
    "type": "enhancement"
}

cloudy-astrophysics / bug-tracker-migration-test

update O III to new storey / badnell paper (trac #293) #295