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A theoretical study is made of the rate at which free atoms form molecules by radiative association. Previous treatments of this problem are shown to be in error. A revised formula for the coefficient expressing the rate is derived. Approximate methods of evaluating this formula are discussed; and tables, designed to ease the computational labour, are presented. The methods developed are used to obtain the rate coefficients for |CH, \, CH^+\, N₂^+\, and\, H₂^+| formation as these are of astrophysical or geophysical importance. In the case of |H₂^+| the calculations can be performed with some precision. Free-free radiative collisions between H atoms and H+ ions are also investigated.
D. R. Bates (Fri,) studied this question.