Using Herschel and Planck observations to delineate the role of magnetic fields in molecular cloud structure (Corrigendum)

Juan D. Soler

doi:10.1051/0004-6361/201935779e

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Erratum

This article is an erratum for:
[https://doi.org/10.1051/0004-6361/201935779]

Issue		A&A Volume 635, March 2020


Article Number		C1
Number of page(s)		1
Section		Interstellar and circumstellar matter
DOI		https://doi.org/10.1051/0004-6361/201935779e
Published online		28 February 2020

A&A 635, C1 (2020)

Using Herschel and Planck observations to delineate the role of magnetic fields in molecular cloud structure (Corrigendum)

Juan D. Soler

Max Planck Institute for Astronomy, Königstuhl 17, 69117, Heidelberg, Germany
e-mail: soler@mpia.de

Key words: ISM: general / ISM: magnetic fields / ISM: clouds / dust, extinction / stars: formation / errata, addenda

Erratum for: A&A, 629, A96 (2019), https://doi.org/10.1051/0004-6361/201935779

There was an error in our Eq. (3). The correct equation should be: $V \equiv \frac{\sum_{k}^{N} w_{k} \cos (2 (ϕ_{k} - ϕ_{0}))}{\sum_{k}^{N} \sqrt{{(w_{k})}^{2} / 2}} .$ $\begin{equation*}V\,\equiv\,\frac{\sum^{N}_{k}w_{k}\cos(2(\phi_{k}-\phi_{0}))}{\sum^{N}_{k}\sqrt{(w_{k})^{2}/2}}. \end{equation*}$ (3)

Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (http://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.

Open Access funding provided by Max Planck Society.

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