Free Access
Erratum
This article is an erratum for:
[https://doi.org/10.1051/0004-6361/201117871]


Issue
A&A
Volume 545, September 2012
Article Number C1
Number of page(s) 1
Section Astrophysical processes
DOI https://doi.org/10.1051/0004-6361/201117871e
Published online 10 September 2012

An error occured during the production process. The top panel of Fig. 1 was truncated. The correct Fig. 1 is published on this page.

thumbnail Fig. 1

The coefficients , , , and , as well as and for the Roberts flow, calculated in the second-order correlation approximation, as functions of k ⊥ /kf, where is the effective wavenumber of the flow. Results obtained with kx = ky and or are represented by open squares and dotted lines or by open diamonds and dashed lines, respectively. Results with kx/ky = 0.75 [k ⊥  = (3,4,0)k1] or kx/ky = 5 [k ⊥  = (5,1,0)k1] and k/k ⊥  = 0.2 are indicated by open or filled circles, respectively. Orange and black symbols correspond to the first and second expressions for and in (21) or for in (26).


© ESO, 2012

All Figures

thumbnail Fig. 1

The coefficients , , , and , as well as and for the Roberts flow, calculated in the second-order correlation approximation, as functions of k ⊥ /kf, where is the effective wavenumber of the flow. Results obtained with kx = ky and or are represented by open squares and dotted lines or by open diamonds and dashed lines, respectively. Results with kx/ky = 0.75 [k ⊥  = (3,4,0)k1] or kx/ky = 5 [k ⊥  = (5,1,0)k1] and k/k ⊥  = 0.2 are indicated by open or filled circles, respectively. Orange and black symbols correspond to the first and second expressions for and in (21) or for in (26).

In the text

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