Mixing is easy: New insights for cosmochemical evolution from pre-stellar core collapse

Open Access

Table 1

Initial pre-stellar core properties.

M₀ (M_⊙)	R_out (au)	E_rot/E_grav	Dust size (µm)	Discussion
1	3000	0.007	1	Sect. 3.1, A.1
1	3000	0.01	1	Sects. A.2, A.1
1	5000	0.007	1	Sects. A.3, A.1

3	3000	0.007	1	Sect. 3.2

1	3000	0.007	1, 10, 100	Sect. 4

Notes. Listed above are the pre-stellar core properties for runs with different initial pre-stellar core mass M₀ (M_⊙), outer radius R_out (au), rotational-to-gravitational energy ratio E_mt/E_glav, fixed dust size (µm), and the corresponding discussion section.

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