Surround and Squash: the impact of superbubbles on the interstellar medium in Scorpius–Centaurus OB2

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Table 2

Stars used in the the 3D hydrodynamic simulation.

Sub^a			M_*^d	T_SN^e
UCL	0	−2.27, 3.56, −3.89	60	4.86
UCL	0	−2.27, 3.56, −3.89	32	7.22
UCL	0	−2.27, 3.56, −3.89	25	8.61
UCL	0	−2.27, 3.56, −3.89	20	10.48
UCL	0	−2.27, 3.56, −3.89	20	10.48
UCL	0	−2.27, 3.56, −3.89	15	15.07

LCC	2	−26.6, −47.6, −25.3	60	6.86
LCC	2	−26.6, −47.6, −25.3	25	10.61
LCC	2	−26.6, −47.6, −25.3	15	17.07

USco	10	50.6, 27.5, 6.16	60	14.86

Notes. ^(a)Subgroup name. ^(b)Formation time in Myr. ^(c)Fixed position of the respective star on the grid in pc. ^(d)Mass of the star in solar masses. ^(d)Explosion time of the star in Myr.

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