Table 2
Parameters that can be excluded to reproduce the solar nebula based on Figs. 7, 8, 9, and 10.
| prule Mdisk [M⊙ ] | rc [au ] | γ | vf [cm s−1 ] | Z0 | τf [torb] | αt | ε | Reason |
|---|---|---|---|---|---|---|---|---|
| 0.05 | ≥35 | 1 | 1000 | 0.0134 | 300 | 10−3 | 0.1 | Fails CCKB condition |
| 0.05 | 20 | 1.5 | 1000 | 0.0134 | 300 | 10−3 | 0.1 | Fails CCKB condition |
| 0.05 | 20 | 1 | 1000 | ≤0.03 | 300 | 10−3 | 0.1 | <MMSN; fails Nice disk condition |
| 0.05 | 20 | 1 | 1000 | 0.0134 | <300 | 10−3 | 0.1 | Fails CCKB condition |
| 0.05 | 20 | 1 | 1000 | 0.0134 | 300 | 10−2 | 0.1 | Fails CCKB condition |
| 0.05 | 20 | 1 | 1000 | 0.0134 | 300 | 10−3 | ≤0.03 | <MMSN (for ε ≲ 0.01); |
| Fails Nice disk cond. | ||||||||
| 0.05 | 20 | 1 | 1000 | 0.0134 | 300 | 10−3 | ≳0.3 | Fails CCKB condition |
| 0.02 | 20 | 1 | 100 | 0.0134 | 1000 | 10−4 | 0.03 | <MMSN; fails Nice disk condition |
| 0.05 | 20 | 1 | 100 | 0.0134 | 1000 | 10−4 | 0.03 | <MMSN; fails Nice disk condition |
| 0.1 | ≤10 | 1 | 100 | 0.0134 | 1000 | 10−4 | 0.03 | Fails Nice disk condition |
| 0.1 | ≥35 | 1 | 100 | 0.0134 | 1000 | 10−4 | 0.03 | Fails CCKB condition |
| 0.1 | 20 | 0.5 | 100 | 0.0134 | 1000 | 10−4 | 0.03 | <MMSN |
| 0.1 | 20 | ≥1.2 | 100 | 0.0134 | 1000 | 10−4 | 0.03 | Fails CCKB condition |
| 0.1 | 20 | 1 | <100 | 0.0134 | 1000 | 10−4 | 0.03 | <MMSN |
| 0.1 | 20 | 1 | 100 | ≤0.003 | 1000 | 10−4 | 0.03 | <MMSN; fails Nice disk condition |
| 0.1 | 20 | 1 | 100 | 0.0134 | 0 | 10−4 | 0.03 | Fails CCKB condition |
| 0.1 | 20 | 1 | 100 | 0.0134 | 1000 | ≥10−3 | 0.03 | <MMSN; fails almost every cond. |
| 0.1 | 20 | 1 | 100 | 0.0134 | 1000 | 10−4 | ≤0.01 | <MMSN; fails Nice disk condition |
| 0.1 | 20 | 1 | 100 | 0.0134 | 1000 | 10−4 | ≳0.3 | Fails CCKB condition |
Notes. We cannot exclude values for LX within the range we analyzed. For all the simulations presented in this table, we used LX = 1030 erg s−1. Here we concentrate on three constraints: (1) the CCKB mass constraints, (2) the necessary mass to fulfill the Nice disk condition, (3) and the MMSN mass. In each row we highlight in bold the parameters that deviate from the default values.
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