Table 3

Properties of Type I and Type II protoplanets (see discussion in text).

Run Type ρc Δtc a Rfc Rsc Mfc Nfc Msc Jfc Jsc
(g cm−3) (kyr) (AU) (AU) (R) (Mj) (105) (Mj) (cm2 s−1 × 1018)
01 IIb 8.5 × 10−9 0.4 49 6.6 9.5 2.3 0.22 0.46 59
02 IIb 1.8 × 10−7 0.3 24 2.3 6.5 1.6 0.21 0.48 18

04 IIb 6.0 × 10−8 0.8 104 14 9.0 1.6 0.12 0.60 32
05 Ia 10−3 1.0 27 3.2 7.3 9.2 1.6 2.6 0.12 0.80 0.07 0.95 21 0.3
06 Ia 10−3 0.3 32 4.5 28 21 3.6 11 0.06 0.92 0.05 0.96 25 2.6

07 Ia 10−3 0.7 27 3.7 5.8 10 1.5 2.8 0.08 0.86 0.05 1.02 18 0.2
08 Ia 10−3 0.1 14 3.2 5.5 6.0 0.9 2.9 0.05 0.90 0.04 1.06 4.1 0.2
09 Ia 10−3 1.1 105 7.1 6.1 13 1.8 5.0 0.08 0.88 0.06 0.99 24 0.5

10 IIb 7.1 × 10−7 0.6 38 4.2 9.5 1.8 0.10 0.67 25
11 Ia 10−3 0.3 24 2.3 5.9 6.9 1.3 2.4 0.10 0.84 0.06 0.99 10 0.2

13 IIa 3.1 × 10−6 0.3 69 2.7 29 14 2.2 5.3 0.08 0.79 0.04 1.17 20 1.4
14 Ib 10−3 0.2 18 2.8 6.1 0.9 0.10 0.86 4.3

16 Ib 10−3 0.4 63 6.5 21 2.8 0.11 0.82 60
17 Ia 10−3 0.5 51 4.5 8.8 11 1.4 2.6 0.13 0.78 0.08 0.93 26 0.2
18 Ib 10−3 1.0 72 1.0 15 1.8 0.09 0.90 16

22 Ia 10−3 0.6 40 3.1 6.4 9.7 1.3 3.5 0.07 0.87 0.04 1.05 10 0.2
23 Ib 10−3 0.3 33 3.2 8.9 1.2 0.11 0.82 12

25 Ib 10−3 0.6 49 6.2 16 1.8 0.11 0.83 46
26 Ia 10−3 0.3 46 5.1 5.5 5.6 0.6 1.9 0.07 0.86 0.04 1.00 7.7 0.1
27 Ia 10−3 1.7 79 8.9 7.6 17 1.7 4.9 0.10 0.86 0.09 0.94 49 0.5

Notes. We list the Run ID, the type of protoplanet, the density at the centre of the protoplanet ρc, the time Δtc it took the protoplanet to collapse from density 10−9g cm−3 to its final central density, the distance of the protoplanet from the star, a, the first and second hydrostatic core radii (Rfc and Rsc, respectively), the first and second hydrostatic core masses (Mfc and Msc, respectively), the number of SPH particles of the first core, which is indicative of how well the first core and its collapse are resolved, the ratios of rotational-to-gravitational βrot and thermal-to-gravitational energies αtherm, for the first and second cores, and finally the specific angular momenta of the first and second cores.

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