EDP Sciences
Free Access
Volume 547, November 2012
Article Number A43
Number of page(s) 16
Section Galactic structure, stellar clusters and populations
DOI https://doi.org/10.1051/0004-6361/201218767
Published online 26 October 2012

Online material

thumbnail Fig. A.1

Setup 2-DD. Time evolution of the column density and the equipotential distribution. Contours as in Fig 2. From top to bottom, on the lefthand side the panels show snapshots at 0, 20, 30, 40, and 50 Myr and on the righthand at 60, 70, 80, 90, and 100 Myr after the simulation onset.

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thumbnail Fig. A.2

Setup 2 with (red contour lines) and without a DM halo (black contour lines) at a maximum refinement level of 6. In the top left panel the contour lines represent the column density distribution log (NHI) = 18.8   ...   21.2   Hcm-2 in 0.6 dex after 100 Myr of simulation time. For the line-of-sight plots in the panels on the right side and the panel at the bottom left, contour lines are at log (NHI) = 18,   19,   20,and21   H   cm-2. The angle α determines the inclination of the line of sight, for details see caption of Fig. 4.

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thumbnail Fig. A.3

As in Fig. A.2 but for Setup 2-D.

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thumbnail Fig. A.4

As in Fig. A.2 but for Setup 3.

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thumbnail Fig. A.5

As in Fig. A.2 but for Setup 3-D.

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© ESO, 2012

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