Episodic accretion in binary protostars emerging from self-gravitating solar mass cores

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Table 1

Summary of the initial physical parameters and the final outcome of the models discussed in this paper.

Model	A	T₀ (K)	Final outcome
M1	0.005	8	Single bound VLM triplet, two bound VLM binaries, single bound VLM star
M2	0.05	8	One bound VLM binary, two single bound VLM stars
M3	0.1	8	Two bound VLM binaries, single bound VLM star
M4	0.2	8	Single bound triplet, single bound VLM star
M5	0.05	10	Two bound VLM binaries
M6	0.05	12	Single bound VLM binary, single bound VLM star

Notes. The initial radius, mass, average density, and rate of rotation for each model are given by the constant values 5 × 10¹⁶ cm, 1 M_⊙, 3.8 × 10⁻¹⁸ g cm⁻³ and 5.0 × 10⁻¹³ rad s⁻¹, respectively.

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