Planet formation around M dwarfs via disc instability - Fragmentation conditions and protoplanet properties

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Fig. 8

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Surface density plots for a selection of discs at the time of fragmentation (i.e. when a density of 10⁻⁹ g cm⁻³ is reached). The fragments are shown by the white points. The initial conditions for each run can be found in Table 1 and the results in Table 2.

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