Abstract
Effective collision strengths for forbidden transitions among the five energetically lowest fine-structure levels of O ii are calculated in the Breit-Pauli approximation using the R-matrix method. Results are presented for the electron temperature range 100-100 000 K. The accuracy of the calculations is evaluated via the use of different types of radial orbital sets and a different configuration expansion basis for the target wavefunctions. A detailed assessment of previous available data is given, and erroneous results are highlighted. Our results reconfirm the validity of the original Seaton and Osterbrock scaling for the optical O ii ratio, a matter of some recent controversy. Finally, we present plasma diagnostic diagrams using the best collision strengths and transition probabilities.
Original language | English |
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Pages (from-to) | 903-912 |
Number of pages | 10 |
Journal | Monthly Notices of the Royal Astronomical Society |
Volume | 397 |
Issue number | 2 |
DOIs | |
State | Published - Aug 2009 |
Keywords
- Atomic data
- Atomic processes
- Line: formation
- Planetary nebulae: general
ASJC Scopus subject areas
- Astronomy and Astrophysics
- Space and Planetary Science