Episodic outbursts during brown dwarf formation | Astronomy & Astrophysics (A&A)

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Table 3

Simulation parameters for low-mass star formation.

run	Ṁ_BGR (M_⊙ yr⁻¹)	α_MRI	α_thermal	β_rot
8	10⁻⁷	0.01	0.39	0.01
9	10⁻⁷	0.1	0.39	0.01
10	10⁻⁷	0.3	0.39	0.01
11	–	–	0.39	0.01

Notes. Ṁ_BGR is the quiescent accretion rate onto the forming protostar, and α_MRI is the viscosity α-parameter for the MRI. α_thermal is the initial thermal to gravitational energy and β_rot is the initial rotational to gravitational energy.

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