English

Electron Impact Excitation of O III: An Assessment

Atomic Physics 2021-03-04 v1 Solar and Stellar Astrophysics

Abstract

Tayal and Zatsarinny [Astrophys. J. 850 (2017) 147] have reported results for energy levels, radiative rates (A-values), lifetimes, and effective collision strengths (Υ\Upsilon) for transitions among 202 levels of C-like O~III. For the calculations they have adopted the multi-configuration Hartree-Fock (MCHF) code for the energy levels and A-values, and B-spline RR-matrix (BSR) code for Υ\Upsilon. Their reported results cover a (much) larger range of levels/transitions than generally available in the literature, and appear to be accurate for energy levels and A-values. However, the magnitude and behaviour of Υ\Upsilon do not appear to be correct for several transitions. We demonstrate this through our independent calculations by adopting the flexible atomic code (FAC) and recommend a fresh calculation for this important ion.

Keywords

Cite

@article{arxiv.2103.02581,
  title  = {Electron Impact Excitation of O III: An Assessment},
  author = {K M Aggarwal},
  journal= {arXiv preprint arXiv:2103.02581},
  year   = {2021}
}

Comments

12 pages of text including 11 figures