Fast methods for tracking grain coagulation and ionization - III. Protostellar collapse with non-ideal MHD

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Table 1

Parameters of the protostellar collapse simulations.

Name	α	R (au)	M (M_⊙)	ρ₀ (g cm⁻³)	B (µG)	t_fc (kyr)	Coagulation
C-3	0.3	2946	1	5.49 × 10⁻¹⁸	133	~30	Yes
C-3-M5	0.3	14738	5	2.19 × 10⁻¹⁹	27	~150	Yes
C-4	0.4	3930	1	2.31 × 10⁻¹⁸	75	~47	Yes
NC-3	0.3	2946	1	5.49 × 10⁻¹⁸	133	~30	No

Notes. Columns are: name of the simulation, thermal over gravitational energy ratio α, radius R, mass M, initial density, ρ₀, and initial magnetic field B of the initial cloud, formation time of the first hydrostatic core, t_fc, and use of coagulation.

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