Table 3
HDUST parameters in the BeAtlas grid.
| Parameter | Value |
|---|---|
| Spectral type | B0.5, B1, B1.5, B2, B2.5, B3, B4, B5, B6, B7, B8 |
| M⋆ (M⊙) | 14.6, 12.5, 10.8, 9.6, 8.6, 7.7, 6.4, 5.5, 4.8, 4.2, 3.8 |
| i (deg) | 0.0, 27.3, 38.9, 48.2, 56.3, 63.6, 70.5, 77.2, 83.6, 90.0 |
| Oblateness (Req∕Rp) | 1.1, 1.2, 1.3, 1.4, 1.45 |
| Σ0 (g cm−2) (a) | 0.02, 0.05, 0.12, 0.28, 0.68, 1.65, 4.00 |
| m(b) | 3.0, 3.5, 4.0, 4.5 |
Notes. First row indicates the spectral type corresponding to the stellar mass (Townsend et al. 2004). Models are calculated with the following fixed parameters: fraction of H in the core Xc = 0.30, metallicity Z = 0.014, and disk radius = 50 Req. (a) Surface density at the base of the disk. (b)Disk mass density law exponent.
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