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Table 2:

The properties of the ram pressure and the surrounding gas of the simulations.
  $v_{\rm {rel}}$ $\rho_{\rm {sur}}$ particle p
run [km s-1] [g/cm3] number [dyn cm-2]
1 1000 $1\times10^{-28}$ $1.08\times10^{6}$ $1.00\times10^{-12}$
2 1000 $5\times10^{-28}$ $5.40\times10^{6}$ $5.00\times10^{-12}$
3 1000 $1\times10^{-27}$ $1.08\times10^{7}$ $1.00\times10^{-11}$
4 1000 $5\times10^{-27}$ $5.40\times10^{7}$ $5.00\times10^{-11}$
5 500 $1\times10^{-28}$ $1.08\times10^{6}$ $2.50\times10^{-13}$
6 500 $5\times10^{-28}$ $5.40\times10^{6}$ $1.25\times10^{-12}$
7 500 $1\times10^{-27}$ $1.08\times10^{7}$ $2.50\times10^{-12}$
8 500 $5\times10^{-27}$ $5.40\times10^{7}$ $1.25\times10^{-11}$
9 100 $1\times10^{-28}$ $1.08\times10^{6}$ $1.00\times10^{-14}$
10 100 $5\times10^{-28}$ $5.40\times10^{6}$ $5.00\times10^{-14}$
11 100 $1\times10^{-27}$ $1.08\times10^{7}$ $1.00\times10^{-13}$
12 100 $5\times10^{-27}$ $5.40\times10^{7}$ $5.00\times10^{-13}$
$v_{\rm {rel}}$: relative velocity between the surrounding gas and the galaxy;
$\rho_{\rm {sur}}$: surrounding gas density; p: ram pressure on the galaxy.

Source LaTeX | All tables | In the text

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