| Issue |
A&A
Volume 562, February 2014
|
|
|---|---|---|
| Article Number | A1 | |
| Number of page(s) | 39 | |
| Section | Extragalactic astronomy | |
| DOI | https://doi.org/10.1051/0004-6361/201322395 | |
| Published online | 29 January 2014 | |
Online material
Appendix A: Simulations maps
 |
Fig. A.1
Orthographic projections of the G1 simulation. Two distinct perpendicular line-of-sights are displayed using two sets of four columns. The edge-on view is displayed in the four left columns, and the face-on view is displayed in the four right columns. The projection angles are kept constant with respect to the original Cartesian axes. For each projection, we show the mass-weighted mean gas density (first column), the mass-weighted mean gas temperature (second column), the mass-weighted mean gas radial velocity (third column), and a mock SDSS u/g/r composite image (fourth column). The gas density, gas temperature, and the velocity range are displayed on the right side of each figure. |
| Open with DEXTER | |
 |
Fig. A.2
Same as Fig. A.1 for simulation G2. |
| Open with DEXTER | |
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Fig. A.3
Same as Fig. A.1 for simulation G3. |
| Open with DEXTER | |
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Fig. A.4
Same as Fig. A.1 for simulation G1_G1_90_0_90. |
| Open with DEXTER | |
 |
Fig. A.5
Same as Fig. A.1 for simulation G1_G1_90_90_0. |
| Open with DEXTER | |
 |
Fig. A.6
Same as Fig. A.1 for simulation G1_G1_90_90_180. |
| Open with DEXTER | |
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Fig. A.7
Same as Fig. A.1 for simulation G1_G1_90_90_90. |
| Open with DEXTER | |
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Fig. A.8
Same as Fig. A.1 for simulation G1_G2_90_0_90. |
| Open with DEXTER | |
 |
Fig. A.9
Same as Fig. A.1 for simulation G1_G2_90_90_0. |
| Open with DEXTER | |
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Fig. A.10
Same as Fig. A.1 for simulation G1_G2_90_90_180. |
| Open with DEXTER | |
 |
Fig. A.11
Same as Fig. A.1 for simulation G1_G2_90_90_90. |
| Open with DEXTER | |
 |
Fig. A.12
Same as Fig. A.1 for simulation G1_G3_90_0_90. |
| Open with DEXTER | |
 |
Fig. A.13
Same as Fig. A.1 for simulation G1_G3_90_90_0. |
| Open with DEXTER | |
 |
Fig. A.14
Same as Fig. A.1 for simulation G1_G3_90_90_180. |
| Open with DEXTER | |
 |
Fig. A.15
Same as Fig. A.1 for simulation G1_G3_90_90_90. |
| Open with DEXTER | |
 |
Fig. A.16
Same as Fig. A.1 for simulation G2_G2_90_0_90. |
| Open with DEXTER | |
 |
Fig. A.17
Same as Fig. A.1 for simulation G2_G2_90_90_0. |
| Open with DEXTER | |
 |
Fig. A.18
Same as Fig. A.1 for simulation G2_G2_90_90_180. |
| Open with DEXTER | |
 |
Fig. A.19
Same as Fig. A.1 for simulation G2_G2_90_90_90. |
| Open with DEXTER | |
 |
Fig. A.20
Same as Fig. A.1 for simulation G2_G3_90_0_90. |
| Open with DEXTER | |
 |
Fig. A.21
Same as Fig. A.1 for simulation G2_G3_90_90_0. |
| Open with DEXTER | |
 |
Fig. A.22
Same as Fig. A.1 for simulation G2_G3_90_90_180. |
| Open with DEXTER | |
 |
Fig. A.23
Same as Fig. A.1 for simulation G2_G3_90_90_90. |
| Open with DEXTER | |
© ESO, 2014
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