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Erratum
This article is an erratum for:
[https://doi.org/10.1051/0004-6361/201323293]

Issue
A&A
Volume 568, August 2014
Article Number C1
Number of page(s) 3
Section Interstellar and circumstellar matter
DOI https://doi.org/10.1051/0004-6361/201323293e
Published online 28 August 2014

Erratum for: A&A 566, A45 (2014), DOI: 10.1051/0004-6361/201323293

Errors occurred during the production process. Figures 4, 16, 18, and 20 were published twice. The correct Figs. 3, 4, 15, 16, 17, 18, 19, and 20 are published below.

Thumbnail: Fig. 3 Refer to the following caption and surrounding text. Fig. 3

Relationship between submillimeter optical-depth and NIR extinction in Orion A. The best linear fit, used to calibrate the data, is shown together with the expected 3σ region, as calculated from direct error propagation in the extinction map.

Thumbnail: Fig. 4 Refer to the following caption and surrounding text. Fig. 4

Same as Fig. 3 for Orion B.

Thumbnail: Fig. 15 Refer to the following caption and surrounding text. Fig. 15

Integral area-extinction relation for Orion A, i.e., the physical cloud area above a given extinction threshold (top panel), and the logarithmic derivative of this quantity (bottom panel). The solid black line shows the result for the entire field, while the solid gray line shows the region covered by Herschel alone. For comparison we also plot as a dashed gray line the same quantity as obtained from the 2MASS/Nicest extinction map and a simple S( >AK)∝AK-2Mathematical equation: \hbox{$A_K) \propto A_K^{-2}$} relation as a red line.

Thumbnail: Fig. 16 Refer to the following caption and surrounding text. Fig. 16

Same as Fig. 15 for Orion B.

Thumbnail: Fig. 17 Refer to the following caption and surrounding text. Fig. 17

Function − S′(>AK), that is, the probability distribution function (pdf) of the measured column densities for Orion A. In this log–log plot a log-normal distribution would appear as a parabola, and a power law as a straight line. The red line shows the slope of the power law −S′(AK)∝AK-3Mathematical equation: \hbox{$-S'(A_K) \propto A_K^{-3}$}.

Thumbnail: Fig. 18 Refer to the following caption and surrounding text. Fig. 18

Same as Fig. 17 for Orion B.

Thumbnail: Fig. 19 Refer to the following caption and surrounding text. Fig. 19

Integral mass-extinction relation for Orion A, i.e. the cloud mass above a given extinction threshold. The color codes follow the same convention as in Fig. 15.

Thumbnail: Fig. 20 Refer to the following caption and surrounding text. Fig. 20

Same as Fig. 19 for Orion B.


© ESO, 2014

All Figures

Thumbnail: Fig. 3 Refer to the following caption and surrounding text. Fig. 3

Relationship between submillimeter optical-depth and NIR extinction in Orion A. The best linear fit, used to calibrate the data, is shown together with the expected 3σ region, as calculated from direct error propagation in the extinction map.
In the text
Thumbnail: Fig. 4 Refer to the following caption and surrounding text. Fig. 4

Same as Fig. 3 for Orion B.
In the text
Thumbnail: Fig. 15 Refer to the following caption and surrounding text. Fig. 15

Integral area-extinction relation for Orion A, i.e., the physical cloud area above a given extinction threshold (top panel), and the logarithmic derivative of this quantity (bottom panel). The solid black line shows the result for the entire field, while the solid gray line shows the region covered by Herschel alone. For comparison we also plot as a dashed gray line the same quantity as obtained from the 2MASS/Nicest extinction map and a simple S( >AK)∝AK-2Mathematical equation: \hbox{$A_K) \propto A_K^{-2}$} relation as a red line.
In the text
Thumbnail: Fig. 16 Refer to the following caption and surrounding text. Fig. 16

Same as Fig. 15 for Orion B.
In the text
Thumbnail: Fig. 17 Refer to the following caption and surrounding text. Fig. 17

Function − S′(>AK), that is, the probability distribution function (pdf) of the measured column densities for Orion A. In this log–log plot a log-normal distribution would appear as a parabola, and a power law as a straight line. The red line shows the slope of the power law −S′(AK)∝AK-3Mathematical equation: \hbox{$-S'(A_K) \propto A_K^{-3}$}.
In the text
Thumbnail: Fig. 18 Refer to the following caption and surrounding text. Fig. 18

Same as Fig. 17 for Orion B.
In the text
Thumbnail: Fig. 19 Refer to the following caption and surrounding text. Fig. 19

Integral mass-extinction relation for Orion A, i.e. the cloud mass above a given extinction threshold. The color codes follow the same convention as in Fig. 15.
In the text
Thumbnail: Fig. 20 Refer to the following caption and surrounding text. Fig. 20

Same as Fig. 19 for Orion B.
In the text

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