Issue |
A&A
Volume 569, September 2014
|
|
---|---|---|
Article Number | A31 | |
Number of page(s) | 23 | |
Section | Cosmology (including clusters of galaxies) | |
DOI | https://doi.org/10.1051/0004-6361/201323362 | |
Published online | 15 September 2014 |
Online material
Appendix A
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Fig. A.1
Dark matter density x-projections in g / cm2 of all 12 clusters. All plots show the inner 5 Mpc/h and use the same color scheme, see Fig. l. |
Open with DEXTER |
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Fig. A.2
Temperature x-projections of all 12 clusters. All plots show the inner 5 Mpc/h and use the same color scheme, see Fig. l. |
Open with DEXTER |
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Fig. A.3
Baroclinic vorticity magnitude x-projections of all 12 clusters. All plots show the inner 5 Mpc/h and use the same color scheme, see Fig. l. The visibility of the grid refinement boundary is due to the usage of a common stencil when calculating the gradient or rotation on the grid data. |
Open with DEXTER |
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Fig. A.4
X-ray emissivity-weighted galactic wind metal mass-fraction x-projection of all 12 clusters. All plots show the inner 5 Mpc/h and use the same color scheme, see Fig. l. |
Open with DEXTER |
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Fig. A.5
X-ray emissivity-weighted ram-pressure-stripped metal mass-fraction x-projection of all 12 clusters. All plots show the inner 5 Mpc/h and use the same color scheme, see Fig. l. |
Open with DEXTER |
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Fig. A.6
X-ray emissivity-weighted total metal mass-fraction x-projection of all 12 clusters. All plots show the inner 2.5 Mpc/h and use the same color scheme, see Fig. l. The color scheme represents a range from 0.2−2 Z⊙ . |
Open with DEXTER |
© ESO, 2014
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