HD | Sp. type1 | Distance2 | Sep.3 | V4 | ![]() |
![]() |
Mass7 | Age8 |
(pc) | (AU) | (mag) | (mag) | (erg/s) | (
![]() |
Myr | ||
560 B | G5 + B9 | 100 ![]() |
770 | 10.37 | 0.00 | 30.56 | 0.95 | 20/30/36/30 |
17543 B | F8 + B6 | 187 ![]() |
4625 | 10.73 | 0.21 | 30.17 | 1.18 | 24/28/-/25 |
23793 B | F3 + B3 | 173 ![]() |
1557 | 9.41 | 0.08 | 30.25 | - | <28* |
27638 B | G2 + B9 | 82 ![]() |
1558 | 8.43 | 0.00 | <28.49 | 1.25 | 12/15/19/15 |
33802 B | G8 + B8 | 74 ![]() |
940 | 9.92 | 0.01 | 30.03 | 0.90 | 25/50/47/37 |
38622 C | G2 + B2 | 245 ![]() |
6125 | 12.01 | 0.04 | 29.99 | 1.05 | 30/100/-/110 |
40494 B | G8 + B3 | 263 ![]() |
8889 | 12.66 | 0.00 | <28.57 | 0.94 | 35/100/-/76 |
53191 B | G3 + A0 | 207 ![]() |
3519 | 11.75 | 0.05 | 29.53 | 1.00 | 30/80/-/39 |
60102 B | G8 + B9.5 | 206 ![]() |
3378 | 11.86 | 0.22 | 30.62 | 1.00 | 15/25/-/20 |
86388 B | F5 + B9 | 177 ![]() |
1628 | 9.98 | 0.02 | 29.42 | 1.28 | -/30/-/110 |
90972 B | F9 + B9.5 | 147 ![]() |
1617 | 9.65 | 0.03 | 30.11 | 1.25 | 14/18/18/15 |
108767 B | K2 + B9 | 27 ![]() |
648 | 8.43 | 0.00 | 28.95 | 0.8 | 40/90/-/93 |
109573 B+ | M2.5 + A0 | 67 ![]() |
509 | 13.3 | 0.00 | 29.75 | 0.3 | 10 |
113703 B | K0 + B4 | 127 ![]() |
1448 | 10.8 | 0.00 | 30.22 | 0.98 | 15/25/19/23 |
113791 B | F7 + B2 | 126 ![]() |
3163 | 9.38 | 0.00 | 29.98 | 1.22 | 18/22/11/21 |
127304 B | K1 + A0 | 106 ![]() |
2734 | 11.37 | 0.04 | <28.73 | 0.84 | 50/100/-/100 |
129791 B | K5 + B9.5 | 129 ![]() |
4554 | 12.93 | 0.26 | 29.82 | - | 39* |
143939 B | K3 + B9 | 167 ![]() |
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. |