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Table 3

Scaling relations between various disc and stellar parameters for a cluster of discs at 2 and 3 Myr.

1 Myr 2 Myr 3 Myr
0.9 0.9
1.4 4.1
1.4 1.4
1.4 1.4

Notes. The values indicate the slope, a, of the power law.

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