= Fine-structure collision strengths and line ratios for Ne V in infrared and optical sources by Michael Dance and others
{c}
{tag=Work by Michael Dance}
{tag=Work by Ethan Palay}
{tag=Work by Sultana N. Nahar}
{tag=Work by Anil K. Pradhan}
{title2=2013}
{title2=10.1093/mnras/stt1398}
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.
https://academic.oup.com/mnras/article/435/2/1576/1042586
https://doi.org/10.1093/mnras/stt1398
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.
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