Table 1: Stellar properties of the selected sample of Lindroos PTTSs.

HD
Sp. type1 Distance2 Sep.3 V4 $A_{\rm v}$5 $\log~L_{\rm X}$6 Mass7 Age8
    (pc) (AU) (mag) (mag) (erg/s) ( $M_{\rm\odot}$) Myr

560 B
G5 + B9 100 $\pm$ 9 770 10.37 0.00 30.56 0.95 20/30/36/30
17543 B F8 + B6 187 $\pm$ 37 4625 10.73 0.21 30.17 1.18 24/28/-/25
23793 B F3 + B3 173 $\pm$ 31 1557 9.41 0.08 30.25 - <28*
27638 B G2 + B9 82 $\pm$ 8 1558 8.43 0.00 <28.49 1.25 12/15/19/15
33802 B G8 + B8 74 $\pm$ 4 940 9.92 0.01 30.03 0.90 25/50/47/37
38622 C G2 + B2 245 $\pm$ 54 6125 12.01 0.04 29.99 1.05 30/100/-/110
40494 B G8 + B3 263 $\pm$ 38 8889 12.66 0.00 <28.57 0.94 35/100/-/76
53191 B G3 + A0 207 $\pm$ 25 3519 11.75 0.05 29.53 1.00 30/80/-/39
60102 B G8 + B9.5 206 $\pm$ 25 3378 11.86 0.22 30.62 1.00 15/25/-/20
86388 B F5 + B9 177 $\pm$ 21 1628 9.98 0.02 29.42 1.28 -/30/-/110
90972 B F9 + B9.5 147 $\pm$ 16 1617 9.65 0.03 30.11 1.25 14/18/18/15
108767 B K2 + B9 27 $\pm$ 9 648 8.43 0.00 28.95 0.8 40/90/-/93
109573 B+ M2.5 + A0 67 $\pm$ 3 509 13.3 0.00 29.75 0.3 10
113703 B K0 + B4 127 $\pm$ 12 1448 10.8 0.00 30.22 0.98 15/25/19/23
113791 B F7 + B2 126 $\pm$ 13 3163 9.38 0.00 29.98 1.22 18/22/11/21
127304 B K1 + A0 106 $\pm$ 8 2734 11.37 0.04 <28.73 0.84 50/100/-/100
129791 B K5 + B9.5 129 $\pm$ 16 4554 12.93 0.26 29.82 - 39*
143939 B K3 + B9 167 $\pm$ 27 1436 11.80 0.00 30.52 1.15 2.5/7/8.3/6
Notes: 1. Adopted from Pallavicini et al. (1992). The spectral type of the early-type primary star is also provided; 2. deduced from Hipparcos parallax of the primary star; 3. separation between the stars of the Lindroos binary system using Hipparcos parallax; 4. adopted from Pallavicini et al. (1992); 5. adopted from L86; 6. adopted from Huélamo et al. (2000); 7. masses estimated adopted from Gerbaldi et al. (2001) using Palla & Stahler (1999) evolutionary tracks; 8. ages adopted from Gerbaldi at al. (2001). The four entries correspond to the ages computed with D'Antona & Mazzitelli (1998), Palla & Stahler (1999), Siess et al. (2000) and Tout et al. (1999) evolutionary tracks, respectively; + data from Webb et al. (1999); * ages adopted from L86; - data not available.

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