Abstract
Photoabsorption by systems of hydrogen atoms and protons in the solar photosphere is studied. Analytical formulas for the partial cross sections for photodissociation of the H +2 molecular ion are derived for the cases of fixed vibrational-rotational energy levels and averaging over a Boltzmann distribution for a given temperature. The photoabsorption coefficients for bound-free and free-free transitions of H-H+ in the solar photosphere are calculated. These are compared with the absorption coefficients for photo-ejection of an electron from a negative hydrogen ion H− and free-free transitions of an electron in the field of a hydrogen atom H. Results can be applied to the Sun and hotter stars.
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Translated from Astronomicheski\(\overset{\lower0.5em\hbox{$\smash{\scriptscriptstyle\smile}$}}{l} \) Zhurnal, Vol. 77, No. 5, 2000, pp. 390–400.
Original Russian Text Copyright © 2000 by Lebedev, Presnyakov, Sobel’man.
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Lebedev, V.S., Presnyakov, L.P. & Sobel’man, I.I. Photodissociative absorption by H +2 in the solar photosphere. Astron. Rep. 44, 338–347 (2000). https://doi.org/10.1134/1.163856
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DOI: https://doi.org/10.1134/1.163856