 Fine-structure collision strengths and line ratios for Ne V in infrared and optical sources by Michael Dance and others

By Michael Dance, Ethan Palay, Sultana N. Nahar and Anil K. Pradhan. Monthly Notices of the Royal Astronomical Society 435(2), 1576–1581; published online 26 August 2013.

Cited passages: section 2.3, equations (3)–(4), Maxwellian effective collision strength and excitation coefficient; section 3.1, low-energy resonance structure and its effect on thermal rates. The published title encloses Ne V in square brackets to denote forbidden lines.