Table 5
Statistical results.
| Sample | Nstars | p | ρ | ppc | ρpc |
|---|---|---|---|---|---|
| HAeBes | 43 | 3 × 10−9 | 0.8 | 4 × 10−3 | 0.4 |
| HAeBes (d < 250 pc) | 19 | 0.09 | 0.4 | 0.06 | 0.4 |
| HAeBes (250 pc < d < 1000 pc) | 19 | 0.2 | 0.4 | 0.2 | 0.3 |
| HAeBes (d > 1000 pc) | 5 | 0.1 | 0.9 | 0.1 | 0.9 |
| TTs | 14 | 0.4 | −0.3 | 0.6 | −0.2 |
| TTs & HAeBes (d < 250 pc) | 33 | 9 × 10−6 | 0.7 | 7 × 10−6 | 0.7 |
Notes. Spearman’s probability of false correlation (p) and correlation coefficient (ρ) between log L* (L⊙) and log rin (au) for the samples and number of stars indicated in the first two cols. The last two columns are the same quantities derived from partial correlations,i.e., removing the possible common dependence on the distances to the sources. Stars with upper or lower limits for rin have not been considered in the calculations.
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