Issue |
A&A
Volume 593, September 2016
|
|
---|---|---|
Article Number | C1 | |
Number of page(s) | 1 | |
Section | Interstellar and circumstellar matter | |
DOI | https://doi.org/10.1051/0004-6361/201423526e | |
Published online | 30 August 2016 |
Chemical probes of turbulence in the diffuse medium: the TDR model (Corrigendum)
1 LERMA, CNRS UMR 8112, École Normale
Supérieure & Observatoire de Paris, 75005
Paris,
France
e-mail: benjamin.godard@obspm.fr
2 Institut d’Astrophysique Spatiale,
CNRS UMR 8617, Université Paris-Sud, 91405
Orsay,
France
Key words: astrochemistry / turbulence / ISM: molecules / ISM: kinematics and dynamics / ISM: structure / errata, addenda
We have noticed two typos in our original paper. In Sect. 3.1, Eq. (2), which gives the expression of the effective temperature of an ion-neutral reaction, should read (Pineau des Forêts et al. 1986) (1)In Sect. 5.2, the destruction timescale of the CH+ by reaction with H2 should read ~1 yr
. These correct expressions are those that have been used in all the calculations performed in our original paper. These typos have therefore no bearing on the paper results/conclusions.
References
- Pineau des Forêts, G., Flower, D. R., Hartquist, T. W., & Dalgarno, A. 1986, MNRAS, 220, 801 [NASA ADS] [CrossRef] [Google Scholar]
© ESO, 2016
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