Table 3.
Open in new tab

For each of the four calculations, we provide online tables of the stars and brown dwarfs that were formed, numbered by their order of formation, listing the mass of the object at the end of the calculation, the time (in units of the initial cloud free-fall time) at which it began to form (i.e. when a sink particle was inserted), and the accretion rate of the object at the end of the calculation (precision ≈10−7 M⊙ yr−1). The first five lines of the table for the solar metallicity calculation are provided.

Object numberMasstformAccretion rate
(M⊙)(tff)(M⊙ yr−1)
11.37490.72663.18 × 10−5
21.86260.80342.3 × 10−6
32.27320.80460
41.32840.80663.0 × 10−6
52.53110.81204.3 × 10−6
Object numberMasstformAccretion rate
(M⊙)(tff)(M⊙ yr−1)
11.37490.72663.18 × 10−5
21.86260.80342.3 × 10−6
32.27320.80460
41.32840.80663.0 × 10−6
52.53110.81204.3 × 10−6
Table 3.
Open in new tab

For each of the four calculations, we provide online tables of the stars and brown dwarfs that were formed, numbered by their order of formation, listing the mass of the object at the end of the calculation, the time (in units of the initial cloud free-fall time) at which it began to form (i.e. when a sink particle was inserted), and the accretion rate of the object at the end of the calculation (precision ≈10−7 M⊙ yr−1). The first five lines of the table for the solar metallicity calculation are provided.

Object numberMasstformAccretion rate
(M⊙)(tff)(M⊙ yr−1)
11.37490.72663.18 × 10−5
21.86260.80342.3 × 10−6
32.27320.80460
41.32840.80663.0 × 10−6
52.53110.81204.3 × 10−6
Object numberMasstformAccretion rate
(M⊙)(tff)(M⊙ yr−1)
11.37490.72663.18 × 10−5
21.86260.80342.3 × 10−6
32.27320.80460
41.32840.80663.0 × 10−6
52.53110.81204.3 × 10−6
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