EDP Sciences
Free Access
Erratum
This article is an erratum for: [this article]

Issue
A&A
Volume 588, April 2016
Article Number C1
Number of page(s) 1
Section Interstellar and circumstellar matter
DOI https://doi.org/10.1051/0004-6361/201425338e
Published online 21 March 2016

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.

thumbnail Fig. 1

Cooling rates for C60 as a function of the internal energy of the molecule.

Open with DEXTER

Acknowledgments

We acknowledge A. Omont who helped us identify the mistake that caused this corrigendum.


© ESO, 2016

All Figures

thumbnail Fig. 1

Cooling rates for C60 as a function of the internal energy of the molecule.

Open with DEXTER
In the text

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