Top-down formation of fullerenes in the interstellar medium (Corrigendum)
Université de Toulouse, UPS-OMP, IRAP,
2 CNRS, IRAP, 9 Av. colonel Roche, BP 44346, 31028 Toulouse Cedex 4, France
3 Department of Physics, PO Box 64, University of Helsinki, 00014 Helsinki, Finland
4 Institut Utinam, CNRS UMR 6213, OSU THETA, Université de Franche-Comté, 41bis avenue de l’Observatoire, 25000 Besançon, France
Key words: astrochemistry / ISM: molecules / methods: numerical / errata, addenda
A mistake in the Matlab script generating the figure for the cooling rates means that the displayed curve for emission of infrared photons by C60 was incorrect in Fig. 2 of our original paper. The correct figure is presented in Fig. 1 of this corrigendum. The cooling rates originally used in our model were the correct ones, so that the results of our paper and its conclusions remain unchanged.
We acknowledge A. Omont who helped us identify the mistake that caused this corrigendum.
© ESO, 2016