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Table 1

Star and disc initial parameters for all the performed simulations.

Sim M [M] R [R] Rint [au] Rc [au] α Md [M] τ [Myr]
S1 1.0 4.600 4482 0.1 40 10−2 0.03 0.55
S2 1.0 4.600 4482 0.1 40 10−2 0.06 1.02
S3 1.0 4.600 4482 0.1 40 10−2 0.10 1.61
S4 1.0 4.600 4482 0.1 40 10−3 0.03 1.19
S5 1.0 4.600 4482 0.1 40 10−3 0.06 2.80
S6 1.0 4.600 4482 0.1 40 10−3 0.10 7.00
S7 1.0 4.600 4482 0.1 40 10−4 0.03 3.49
S8 1.0 4.600 4482 0.1 40 10−4 0.06 8.04
S9 1.0 4.600 4482 0.1 40 10−4 0.10 >10

S10 1.5 4.105 4797 0.114 51.5 1.5 × 10−2 0.045 0.64
S11 1.5 4.105 4797 0.114 51.5 1.5 × 10−2 0.09 0.97
S12 1.5 4.105 4797 0.114 51.5 1.5 × 10−2 0.15 1.52
S13 1.5 4.105 4797 0.114 51.5 1.5 × 10−3 0.045 1.42
S14 1.5 4.105 4797 0.114 51.5 1.5 × 10−3 0.09 2.65
S15 1.5 4.105 4797 0.114 51.5 1.5 × 10−3 0.15 4.58
S16 1.5 4.105 4797 0.114 51.5 1.5 × 10−4 0.045 5.05
S17 1.5 4.105 4797 0.114 51.5 1.5 × 10−4 0.09 6.10
S18 1.5 4.105 4797 0.114 51.5 1.5 × 10−4 0.15 8.54

S19 2.0 3.882 4797 0.126 61.7 2 × 10−2 0.06 0.66
S20 2.0 3.882 4797 0.126 61.7 2 × 10−2 0.12 0.98
S21 2.0 3.882 4797 0.126 61.7 2 × 10−2 0.20 1.42
S22 2.0 3.882 4797 0.126 61.7 2 × 10−3 0.06 1.38
S23 2.0 3.882 4797 0.126 61.7 2 × 10−3 0.12 2.64
S24 2.0 3.882 4797 0.126 61.7 2 × 10−3 0.20 3.56
S25 2.0 3.882 4797 0.126 61.7 2 × 10−4 0.06 6.40
S26 2.0 3.882 4797 0.126 61.7 2 × 10−4 0.12 7.60
S27 2.0 3.882 4797 0.126 61.7 2 × 104 0.20 9.52

S28 2.5 4.204 5178 0.136 70.9 2.5 × 10−2 0.075 0.57
S29 2.5 4.204 5178 0.136 70.9 2.5 × 10−2 0.15 0.84
S30 2.5 4.204 5178 0.136 70.9 2.5 × 10−2 0.25 1.14
S31 2.5 4.204 5178 0.136 70.9 2.5 × 10−3 0.075 1.14
S32 2.5 4.204 5178 0.136 70.9 2.5 × 10−3 0.15 2.51
S33 2.5 4.204 5178 0.136 70.9 2.5 × 103 0.25 3.65
S34 2.5 4.204 5178 0.136 70.9 2.5 × 10−4 0.075 8.50
S35* 2.5 4.204 5178 0.136 70.9 2.5 × 104 0.15 9.50
S36 2.5 4.204 5178 0.136 70.9 2.5 × 10−4 0.25 >10

S37 3.0 4.571 5415 0.144 79.5 3 × 10−2 0.09 0.42
S38* 3.0 4.571 5415 0.144 79.5 3 × 102 0.18 1.15
S39 3.0 4.571 5415 0.144 79.5 3 × 10−2 0.30 1.23
S40 3.0 4.571 5415 0.144 79.5 3 × 103 0.09 1.70
S41 3.0 4.571 5415 0.144 79.5 3 × 10−3 0.18 2.17
S42 3.0 4.571 5415 0.144 79.5 3 × 10−3 0.30 2.25
S43 3.0 4.571 5415 0.144 79.5 3 × 10−4 0.09 9.75
S44 3.0 4.571 5415 0.144 79.5 3 × 10−4 0.18 >10
S45 3.0 4.571 5415 0.144 79.5 3 × 10−4 0.30 >10

Notes. M denotes the mass of the star, while R and refer to the radius and effective temperature of the star at the birthline, respectively. Rint and Rc represent the inner border and the characteristic radius of the disc, respectively. α is the viscosity parameter and Md the mass of the disc. The last column refers to τ, the disc dissipation timescale, which is not an initial condition but a result of our simulations (see Sect. 3.5). The cases highlighted in bold face are referring to the revenant discs that will be described in Sect. 3.4. Simulations S35* and S38* represent cases that do not strictly follow the revenant disc evolution.

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