Carbon ion

Collisional rate coefficients are taken from the literature and include collisions with H (Barinovs et al 2005), e (Wilson & Bell 2002), and H2 (Lique et al. 2013).

The standard datafile only includes the fine structure transition while a second file includes the principal ultraviolet transitions.

The rates for para-H2 assume thermalized rotational populations in hydrogen and include both H2(J=0) and H2(J=2) as collision partners (Wiesenfeld & Goldsmith 2014).

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