
An accurate set of H3O+ – H2 collisional rate coefficients for non-LTE modelling of warm interstellar clouds (vol 518, pg 3593, 2023)
We have discovered errors in our recent paper Demes et al. (2022). Indeed, the supplementary material contains some incorrect theoretical data due to a software bug in the calculations of high energy cross sections. The cross sections for para-H3O+ collision with ortho-H2 are affected at total energies above 800 cm−1. Consequently, most of the high temperature rate coefficients for the para-H3O+ + ortho-H2 nuclear spin configurations are affected too.
Eredeti fellelhetőség: mtmt.hu


