Table 1.
Stellar and disk parameters.
| Parameters | Symbol | Value |
|---|---|---|
| Stellar Mass | M⋆ | 1 M⊙ |
| Stellar Luminosity | L⋆ | 11.02, 2.17, 0.46 L⊙ |
| Effective temperature | Teff | 4147, 4282, 4290 K |
| UV luminositya | LUV | 0.01 L⊙ |
| X-ray luminositya | LX | 1030 erg s−1 |
| Cosmic ray ionization rate | CRI | 1.7 × 10−17 s−1 |
| Disk mass | Md | 0.003, 0.03 M⊙ |
| Disk inner radius | Rin | 0.07 au |
| Disk outer radius | Rout | 100 au |
| Tapering-off radius | Rtap | 50 au |
| Reference scale height | H0 | 0.4 au |
| Reference radius | Rref | 10 au |
| Dust settling turbulence | α | 0.1 |
| Column density indexa | ϵ | 1.0 |
| Dust-to-gas mass ratioa | ρd/ρg | 0.01 |
| Min. size dust graina | amin | 0.05 μm |
| Max. size dust graina | amax | 3000 μm |
| Dust size distr. indexa | p | 3.5 |
| Dust compositiona: | ||
| Mg0.7Fe0.3SiO3 | 60% | |
| amorph. carbon | 15% | |
| porosity | 25% | |
| Dust material density | ρgr | 2.076 g cm−3 |
Notes. ProDiMo input parameters used to model six early solar nebula, for two disk mass values (0.003 M⊙ and 0.03 M⊙) at three nebular ages (0.2 Myr, 1 Myr, and 10 Myr), to which the following stellar parameters (L⋆ and Teff) correspond respectively (11.02 L⊙, 4147 K), (2.17 L⊙, 4282 K), and (0.46 L⊙, 4290 K).
Standard values from Helling et al. (2014) and Woitke et al. (2009).
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