**Table 1:** Initial conditions for the numerical simulations. $N_{\rm p}$ is the number of particles considered, $r_{\rm {b/d/h}}$ and $M_{\rm {b/d/h}}$ the galaxy bulge/disk/halo radii and masses, and $f_{\rm {el}}$ the collision elasticity factor.
Run	$N_{\rm p}$	$r_{\rm b}$	$M_{\rm b}$	$r_{\rm d}$	$M_{\rm d}$	$r_{\rm h}$	$M_{\rm h}$	$f_{\rm {el}}$
id.	$\times$ 10³	kpc	⁽¹⁾	kpc	⁽¹⁾	kpc	⁽¹⁾
Run 0	100	1.1	2.5	4.4	8.0	16.0	7.2	0.65
Run 1	100	1.1	6.8	4.4	8.0	16.0	11.8	0.65
Run 2	100	1.1	6.8	4.4	8.0	16.0	11.8	0.85
Run 3	400	1.1	6.8	4.4	8.0	16.0	11.8	0.65
Run 4	400	1.1	6.8	4.4	8.0	16.0	11.8	0.85

⁽¹⁾ Masses are in 10 $^{10}~M_{\odot}$ .

Source LaTeX | All tables | In the text