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This is a Quantitative Study study.

Electron impact ro-vibrational transitions and dissociative recombination of H_2^+ and HD^+. Rate coefficients and astrophysical implications

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Newly calculated rate coefficients and cross sections for H2+ and HD+ transitions, suggesting implications for astrochemistry.

Updated thermal rate coefficients show significant differences from previous studies, impacting astrochemical models.
Analysis reveals how electron-induced processes affect the formation of interstellar molecules and cosmic chemistry.
The study provides crucial data for understanding hydrogen-rich plasmas in environments like planetary nebulae.
Incorporating new DR rates leads to substantial changes in predicted molecular abundances in metal-free gas.

Hassaine et al. (2025) studied this question.

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