In this paper we compute the collision strengths and their thermally averaged Maxwellian values for electron transitions between the 15 lowest levels of doubly ionized cobalt, Co2+, which give rise to forbidden emission lines in the visible and infrared region of spectrum. The calculations also include transition probabilities and predicted relative line emissivities. The data are particularly useful for analysing the thermodynamic conditions of supernova ejecta.
CITATION STYLE
Storey, P. J., & Sochi, T. (2016). Collision strengths and transition probabilities for Co III forbidden lines. Monthly Notices of the Royal Astronomical Society, 459(3), 2558–2565. https://doi.org/10.1093/mnras/stw776
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