Free Access
Issue
A&A
Volume 578, June 2015
Article Number A18
Number of page(s) 23
Section Interstellar and circumstellar matter
DOI https://doi.org/10.1051/0004-6361/201424798
Published online 25 May 2015

Online material

thumbnail Fig. 33

Snapshot time sequence of the simulation OPGs with NSM = 1003, showing the smooth formation of a planetoid. The slice size is 0.025 × 1 × 1 L3 at x = (0.5 ± 0.0125)L.

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thumbnail Fig. 34

Snapshot comet mass-distribution sequence of the simulation OPGs with NSM = 1003.

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thumbnail Fig. 35

Snapshot comet mass-distribution sequence of all OPGs simulations with NSM equal to the triangle pointing down: 503, triangle pointing up: 643, square: 803, diamond: 1003, circle: 1283, star: 1603.

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thumbnail Fig. 36

Snapshot comet mass-distribution summation sequence of OPGs simulations. Reference with NSM = 1283: circle; sum of 4 comet sizes per star: 1003.

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thumbnail Fig. 37

0.2 × 1 × 1 L3 snapshots at x = (0.5 ± 0.1)L of simulation PT2-2 with NSM = 503, and without gravity.

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thumbnail Fig. 38

Comet mass-distribution snapshots of simulation PT2-2 with NSM = 503, and without gravity.

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thumbnail Fig. 39

0.025 × 1 × 1 L3 snapshots at x = (0.5 ± 0.0125)L of sufficiently self-gravitating simulation PT1-3 with NSM = 1003.

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thumbnail Fig. 40

Comet mass-distribution snapshots of sufficiently self-gravitating simulation PT1-3 with NSM = 1003.

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thumbnail Fig. 41

0.025 × 1 × 1 L3 snapshots at x = (0.5 ± 0.0125)L of weakly self-gravitating simulation PT2-2 with NSM = 1003.

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thumbnail Fig. 42

Comet mass distribution of weakly self-gravitating simulation PT2-2 with NSM = 1003.

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thumbnail Fig. 43

0.025 × 1 × 1 L3 snapshots at x = (0.5 ± 0.0125)L of weakly self-gravitating simulation PT3-2 with NSM = 1003.

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thumbnail Fig. 44

Comet mass distribution of weakly self-gravitating simulation PT3-2 with NSM = 1003.

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© ESO, 2015

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