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Table 1
Stellar and disk parameters in our hydrodynamical models.
Model No. | m∗(M⊙) | T∗(K) | R∗(R⊙) | i(°) | mp(MJ) |
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#1 | 0.5 | 3760 | 1.4 | 20,40,60 | 0.5 |
#2 | 0.5 | 3760 | 1.4 | 20,40,60 | 1.5 |
#3 | 0.5 | 3760 | 1.4 | 20,40,60 | 2.5 |
#4 | 0.5 | 3760 | 1.4 | 20,40,60 | 4 |
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#5 | 1 | 4266 | 1.83 | 20,40,60 | 1 |
#6 | 1 | 4266 | 1.83 | 20,40,60 | 3 |
#7 | 1 | 4266 | 1.83 | 20,40,60 | 5 |
#8 | 1 | 4266 | 1.83 | 20,40,60 | 8 |
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#9 | 1.5 | 4584 | 2.22 | 20,40,60 | 1.5 |
#10 | 1.5 | 4584 | 2.22 | 20,40,60 | 4.5 |
#11 | 1.5 | 4584 | 2.22 | 20,40,60 | 7.5 |
#12 | 1.5 | 4584 | 2.22 | 20,40,60 | 12 |
Notes. The stellar parameters were taken from a publicly available tool (Siess et al. 2000). The disk extends between 0.2−5 AU and the orbital distance of the massive planets is 1 AU.
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