Table 4
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Set-up of the different simulations. The table lists whether star formation and cooling (SF/cool.) is applied, the number of gas (NGas) and dark matter particles (NDM), the mass of the gas (MGas) and dark matter particles (MDM), as well as the initial magnetic field orientation and strength for all simulated scenarios, respectively.

ScenarioSF/cool.NGasNDMformulaformulaformulaformula (G)
ga0_bx0Yes68 32368 3232.6 × 1071.4 × 108–0
ga0_bx10Yes68 32368 3232.6 × 1071.4 × 108x10−10
ga0_bx14Yes68 32368 3232.6 × 1071.4 × 108x10−14
ga0_bx18Yes68 32368 3232.6 × 1071.4 × 108x10−18
ga0_by18Yes68 32368 3232.6 × 1071.4 × 108y10−18
ga0_bx22Yes68 32368 3232.6 × 1071.4 × 108x10−22
ga0_bx26Yes68 32368 3232.6 × 1071.4 × 108x10−26
ga0_bx30Yes68 32368 3232.6 × 1071.4 × 108x10−30
ga0_bx34Yes68 32368 3232.6 × 1071.4 × 108x10−34
ga1_bx0Yes637 966637 9662.8 × 1061.5 × 107–0
ga1_bx18Yes637 966637 9662.8 × 1061.5 × 107x10−18
ga1_bx18_nosfNo637 966637 9662.8 × 1061.5 × 107x10−18
ga2_bx0Yes5953 0335953 0333.0 × 1051.6 × 106–0
ga2_bx18Yes5953 0335953 0333.0 × 1051.6 × 106x10−18
ScenarioSF/cool.NGasNDMformulaformulaformulaformula (G)
ga0_bx0Yes68 32368 3232.6 × 1071.4 × 108–0
ga0_bx10Yes68 32368 3232.6 × 1071.4 × 108x10−10
ga0_bx14Yes68 32368 3232.6 × 1071.4 × 108x10−14
ga0_bx18Yes68 32368 3232.6 × 1071.4 × 108x10−18
ga0_by18Yes68 32368 3232.6 × 1071.4 × 108y10−18
ga0_bx22Yes68 32368 3232.6 × 1071.4 × 108x10−22
ga0_bx26Yes68 32368 3232.6 × 1071.4 × 108x10−26
ga0_bx30Yes68 32368 3232.6 × 1071.4 × 108x10−30
ga0_bx34Yes68 32368 3232.6 × 1071.4 × 108x10−34
ga1_bx0Yes637 966637 9662.8 × 1061.5 × 107–0
ga1_bx18Yes637 966637 9662.8 × 1061.5 × 107x10−18
ga1_bx18_nosfNo637 966637 9662.8 × 1061.5 × 107x10−18
ga2_bx0Yes5953 0335953 0333.0 × 1051.6 × 106–0
ga2_bx18Yes5953 0335953 0333.0 × 1051.6 × 106x10−18
Table 4
Open in new tab

Set-up of the different simulations. The table lists whether star formation and cooling (SF/cool.) is applied, the number of gas (NGas) and dark matter particles (NDM), the mass of the gas (MGas) and dark matter particles (MDM), as well as the initial magnetic field orientation and strength for all simulated scenarios, respectively.

ScenarioSF/cool.NGasNDMformulaformulaformulaformula (G)
ga0_bx0Yes68 32368 3232.6 × 1071.4 × 108–0
ga0_bx10Yes68 32368 3232.6 × 1071.4 × 108x10−10
ga0_bx14Yes68 32368 3232.6 × 1071.4 × 108x10−14
ga0_bx18Yes68 32368 3232.6 × 1071.4 × 108x10−18
ga0_by18Yes68 32368 3232.6 × 1071.4 × 108y10−18
ga0_bx22Yes68 32368 3232.6 × 1071.4 × 108x10−22
ga0_bx26Yes68 32368 3232.6 × 1071.4 × 108x10−26
ga0_bx30Yes68 32368 3232.6 × 1071.4 × 108x10−30
ga0_bx34Yes68 32368 3232.6 × 1071.4 × 108x10−34
ga1_bx0Yes637 966637 9662.8 × 1061.5 × 107–0
ga1_bx18Yes637 966637 9662.8 × 1061.5 × 107x10−18
ga1_bx18_nosfNo637 966637 9662.8 × 1061.5 × 107x10−18
ga2_bx0Yes5953 0335953 0333.0 × 1051.6 × 106–0
ga2_bx18Yes5953 0335953 0333.0 × 1051.6 × 106x10−18
ScenarioSF/cool.NGasNDMformulaformulaformulaformula (G)
ga0_bx0Yes68 32368 3232.6 × 1071.4 × 108–0
ga0_bx10Yes68 32368 3232.6 × 1071.4 × 108x10−10
ga0_bx14Yes68 32368 3232.6 × 1071.4 × 108x10−14
ga0_bx18Yes68 32368 3232.6 × 1071.4 × 108x10−18
ga0_by18Yes68 32368 3232.6 × 1071.4 × 108y10−18
ga0_bx22Yes68 32368 3232.6 × 1071.4 × 108x10−22
ga0_bx26Yes68 32368 3232.6 × 1071.4 × 108x10−26
ga0_bx30Yes68 32368 3232.6 × 1071.4 × 108x10−30
ga0_bx34Yes68 32368 3232.6 × 1071.4 × 108x10−34
ga1_bx0Yes637 966637 9662.8 × 1061.5 × 107–0
ga1_bx18Yes637 966637 9662.8 × 1061.5 × 107x10−18
ga1_bx18_nosfNo637 966637 9662.8 × 1061.5 × 107x10−18
ga2_bx0Yes5953 0335953 0333.0 × 1051.6 × 106–0
ga2_bx18Yes5953 0335953 0333.0 × 1051.6 × 106x10−18
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