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).

Open with DEXTER


© 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).

Open with DEXTER
In the text

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