Volume 638, June 2020
|Number of page(s)||1|
|Section||Interstellar and circumstellar matter|
|Published online||05 June 2020|
Molecule formation in dust-poor irradiated jets
I. Stationary disk winds (Corrigendum)
Leiden Observatory, Leiden University,
PO Box 9513,
2 LERMA, Observatoire de Paris, PSL Research Univ., CNRS, Sorbonne Univ., 75014 Paris, France
3 Laboratoire de Physique de l’École normale supérieure, ENS, Université PSL, CNRS, Sorbonne Université, Université Paris-Diderot, Sorbonne Paris Cité, 75005 Paris, France
4 Université Paris-Saclay, CNRS, Institut d’Astrophysique Spatiale, 91405 Orsay, France
5 Max-Planck-Institut für Extraterrestrische Physik, Giessenbachstrasse1, 85748 Garching, Germany
Key words: stars: formation / stars: jets / stars: protostars / ISM: molecules / errata, addenda
Some typographical errors occurred during the production process of the original published article. The lines below Eqs. (14) and (15) should read “where we note as…”. Also, in Appendix C, Eqs. (C.15) and (C.16) were switched and the new Eq. (C.16) is not correct. The sentence that contains the two equations should read:
of the XH+ formed by radiative association is converted in H2.
© ESO 2020
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