The Rosetta Stone project - III. ALMA synthetic observations of fragmentation in high-mass star-forming clumps

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Table 1

Initial conditions for the RS1.0 simulations.

Parameter	Available initial conditions
Seed	[1, 2]
M (M_⊙)	[500, 1000]
R (pc)	[0.383]
μ	[3, 10, 100]
M	[7, 10]

Notes. Col. 1: parameters to be set (top to bottom: turbulent seed, mass, radius, mass-to-flux ratio, and Mach number). Col. 2: available initial conditions for each parameter.

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