The Rosetta Stone Project - I. A suite of radiative magnetohydrodynamics simulations of high-mass star-forming clumps

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Table 2

Additional individual runs explored for this study.

Seed	N_jeans	n_sink [cm⁻³]
3	10	10⁹
4	10	10⁹
1	20	10⁹
1	10	10¹⁰

Notes. These runs were all computed with a clump mass of 1000 M_⊙, radius of 0.38 pc, Mach number of 7, and mass-to-flux ratio of 10.

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