Volume 636, April 2020
|Number of page(s)||1|
|Section||Interstellar and circumstellar matter|
|Published online||06 April 2020|
Breakdown curves of CH2(+), CH3(+), and CH4(+) molecules
I. Construction and application to electron collisions and UV photo-dissociation (Corrigendum)
Institut de Physique Nucléaire d’Orsay (IPNO), CNRS, Univ. Paris Sud, Université Paris-Saclay,
91406 Orsay, France
2 Institut des Sciences Moléculaires d’Orsay (ISMO), CNRS, Univ. Paris Sud, Université Paris-Saclay, 91405 Orsay, France
3 Université de Toulouse, UPS-OMP, IRAP, 31028 Toulouse cedex 4, France
4 Departamento de Química, Módulo 13, Condensed Matter Physic Center (IFIMAC), Institute for advanced Research in Chemical Sciences (IAdChem), Universidad Autónoma de Madrid, 28049 Madrid, Spain
Key words: astrochemistry / ISM: molecules / molecular processes / errata, addenda
A typographical error was made in Eq. (1) of the paper, which expresses the relation between the kinetic energy and the radial distribution for the detector, based on the isotropic hypothesis of the collision. The formula should be written as: (1)
We thank Prof. Xavier Urbain for notifying us of the error.
© T. IdBarkach et al. 2020
Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (http://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
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