Environmental effects on the dynamical evolution of star clusters in turbulent molecular clouds

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Volume 667 (November 2022)

A&A, 667 (2022) A69

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Table A.2.

List of SPH simulations of the environment.

Name	V_rms/km s⁻¹	k_kick	N_sph
`V10_k[4-8]`	10	[4, 8]	128³
`V15_k[4-8]_lr`^a	15	[4, 8]	64³
`V15_k[4-8]`^b	15	[4, 8]	128³
`V15_k[4-8]_hr`^a	15	[4, 8]	256³
`V15_k[2-4]`	15	[2, 4]	128³
`V15_k[8-16]`	15	[8,16]	128³
`V20_k[4-8]`	20	[4, 8]	128³
`V40_k[4-8]`	40	[4, 8]	128³

Notes. For each simulation, the following initial conditions are given: the root mean square velocity, the range of the kick wavenumber, and the number of SPH particles. We note that the mean number density is ⟨n⟩=10 cm⁻³ and the simulation box size is L = 400 pc in all models.

Labels “lr” and “hr” identify the low and high resolution runs, respectively.

V15_k[4-8] is the model used in the simulations of star clusters embedded in the environment.

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