http://arxiv.org/abs/1412.2606

The matrix elements and energies needed to calculate vibrational-rotational state resolved cross sections and rate coefficients for radiative association of H and p and for photodissociation of H${}_2^+$ are presented for applications to simulations of chemistry in the early Universe and to stellar atmospheres.

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J. Babb

Tue, 9 Dec 14

21/64

Comments: 8 pages, 1 figure, ApJS accepted

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