Table 5
Comparison to the near-IR interferometry constraints of observed systems.
| Model/star | log10(Ṁ) | L∗ |  |
 |
aH [au] | aK [au] | aL [au] | aN [au] | FN [Jy] |
|---|---|---|---|---|---|---|---|---|---|
| M001 | −8 | 21 | 0.28 | 0.46 | 0.31 | 0.34 | 0.42 | 0.79 | 25.7 |
| M03 | −8 | 21 | 0.3 | 0.51 | 0.34 | 0.42 | 0.49 | 0.93 | 36.2 |
| M001_S_TC | −8 | 21 | 0.40 | 0.62 | 0.24 | 0.24 | 0.25 | 0.79 | 22.0 |
| HD 163296 |  |
15.8 | 0.76 ± 0.01 | 0.81 ± 0.01 | 0.22 ± 0.05 | 0.3 ± 0.01 | 0.33 ±0.01 | 0.82 ± 0.05 | 16.3 ± 0.6 |
| HD 169142 | < −8.7 | 20.4 | 0.17 ± 0.01 | 0.40 ± 0.05 | 0.11 ± 0.02 5 | 0.33 ± 0.07 | – | 9.5 ± 2.3 | 0.92 ± 0.3 |
| HD 100546 | ≈ −7 | 22.5 | 0.42 ± 0.02 | 0.63 ± 0.01 | 0.26 ± 0.01 | 0.28 ± 0.01 | – | 21.3 ± 1.1 | 69.1 ± 1.5 |
Notes. From left to right, we list the model name, the accretion rate in units of M⊙/yr, the stellar luminosity, the fraction of the disk emission in the H and K bands, the half-light radius for the H, K, L, and N bands in units of au, and the N-band flux normalized at 100 pc in units of Jy. The accretion rates were measured using X-Shooter observations and fitting the Hα emission for HD 163296 (Wichittanakom et al. 2020), HD 169142 (Grady et al. 2007), and HD 100546 (Mendigutía et al. 2015). The H-band information on the disk selection was retrieved from Lazareff et al. (2017) Table B.2 and from the CDS Link. The K-band information was taken from GRAVITY Collaboration (2019) Table 3. The L-band information for HD 163296 was taken from Varga et al. (2021). The N-band information was from Menu et al. (2015) Table 2. Gaia DR3 distances were assumed for HD 169142 (114.9 pc), HD 163296 (101 pc), and HD 100546 (110 pc).
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