Table C.2
Parameters of the DUNES_DB stars with d ≤ 15 pc and 15 pc <d ≤ 20 pc.
HIP | Teff | log g | [Fe/H] | Flag | Lbol |
![]() |
Ref. | Prot (d) | t Gyro) | tHK |
(K) | (cm/s2) | (dex) | (L⊙) | or lower limit† | (Gyr) | (Gyr) | ||||
|
||||||||||
FGK stars (d ≤ 15 pc) | ||||||||||
|
||||||||||
1599 | 5960 | 4.45 | −0.17 | S | 1.224 | −4.855 | 1 | 14.01 ± 0.97 | 2.20 | 4.03 |
3765 | 4977 | 4.57 | −0.22 | S | 0.283 | −4.852 | 2 | 39.02 ± 0.25 | 5.41 | 3.98 |
7751 | 4993 | 4.54 | −0.23 | S | 0.304 | −4.94 | 3 | |||
7918 | 5891 | 4.36 | + 0.06 | S | 1.405 | −4.987 | 4 | 21.10 ± 0.12 | 3.56 | 6.36 |
7981 | 5189 | 4.52 | −0.04 | S | 0.439 | −4.912 | 2 | 39.60 ± 0.43 | 6.04 | 4.99 |
10644 | 5684 | 4.36 | −0.45 | P | 1.118 | −4.644 | 4 | 11.57 ± 0.35 | 1.30 | 1.47 |
12114 | 4866 | 4.66 | + 0.00 | S | 0.257 | −4.958 | 2 | 44.90 ± 0.53 | 6.66 | 5.82 |
12843 | 6273 | 4.20 | −0.04 | P | 2.585 | −4.524 | 1 | 2.92 ± 0.36 | 0.71 | |
14879 | 6275 | 4.40 | −0.19 | S | 4.923 | −4.901 | 1 | 11.58 ± 1.39 | 2.12 | 4.79 |
15457 | 5755 | 4.52 | + 0.11 | S | 0.838 | −4.42 | 2 | 7.53 ± 0.18 | 0.46 | 0.35 |
15510 | 5415 | 4.55 | −0.34 | S | 0.637 | −4.998 | 1 | 32.42 ± 0.55 | 5.51 | 6.56 |
16852 | 6014 | 4.08 | −0.06 | S | 3.060 | −5.053 | 4 | 17.06 ± 0.95 | 3.13 | 7.59 |
22449 | 6457 | 4.15 | −0.01 | S | 2.708 | −4.788 | 4 | 5.83 ± 0.18 | 3.04 | |
23693 | 6165 | 4.38 | −0.20 | P | 1.414 | −4.49 | 3 | 3.91 ± 0.37 | 0.40 | 0.57 |
27072 | 6331 | 4.28 | −0.10 | P | 2.291 | −4.817 | 1 | 5.91 ± 0.66 | 3.45 | |
37279 | 6578 | 3.99 | + 0.01 | S | 6.605 | −4.777 | 2 | 3.21 ± 0.59 | 2.89 | |
47080 | 5539 | 4.48 | + 0.33 | S | 0.822 | −4.638 | 2 | 21.86 ± 0.10 | 2.39 | 1.42 |
56997 | 5514 | 4.50 | −0.04 | S | 0.618 | −4.546 | 2 | 14.62 ± 0.65 | 1.31 | 0.82 |
57443 | 5630 | 4.51 | −0.28 | S | 0.806 | −4.957 | 1 | 25.90 ± 0.47 | 4.27 | 5.80 |
57757 | 6125 | 4.12 | + 0.14 | S | 3.483 | −4.99 | 5 | 10.27 ± 1.37 | 2.62 | 6.41 |
59199 | 7042 | 4.21 | −0.14 | P | 4.175 | −5.373 | 6 | >3.26 (21.7) | ||
61317 | 5890 | 4.40 | −0.17 | S | 1.178 | −4.851 | 4 | 15.11 ± 0.89 | 2.32 | 3.96 |
61941 | 6797 | 4.25 | −0.13 | P | 8.346 | −4.50 | 6 | 6.31 ± 0.37‡ | 0.61 | |
64394 | 6065 | 4.43 | + 0.04 | S | 1.381 | −4.745 | 2 | 11.48 ± 0.49 | 1.59 | 2.49 |
64924 | 5646 | 4.57 | + 0.10 | S | 0.820 | −5.001 | 2 | 32.29 ± 0.78 | 5.50 | 6.62 |
70497 | 6315 | 4.29 | −0.10 | P | 4.034 | −4.591 | 4 | 4.26 ± 0.21 | 2.25 | 1.08 |
72659 | 5549 | 4.63 | −0.10 | S | 0.611 | −4.363 | 2 | 6.49 ± 0.31 | 0.31 | 0.23 |
73695 | 5851 | 4.30 | −0.19 | S | 1.552 | −4.602 | 4 | 12.85 ± 0.13 | 1.31 | 1.16 |
77257 | 5899 | 4.17 | + 0.01 | S | 2.077 | −5.004 | 2 | 19.73 ± 0.96 | 3.40 | 6.67 |
78072 | 6265 | 4.08 | −0.15 | S | 2.863 | −5.113 | 4 | >5.2 (11.42) | ||
80686 | 6029 | 4.46 | −0.19 | P | 1.301 | −4.65 | 3 | 8.25 ± 1.00 | 1.02 | 1.52 |
89937 | 6034 | 4.27 | −0.65 | P | 1.942 | −4.9 | 6 | 7.13 ± 0.35 | 4.78 | |
93017 | 5834 | 4.33 | −0.19 | P | 1.515 | −4.874 | 2 | 16.18 ± 0.31 | 2.53 | 4.34 |
99825 | 5105 | 4.48 | −0.03 | S | 0.405 | −5.048 | 1 | 47.33 ± 0.78 | 7.74 | 7.50 |
102485 | 6590 | 4.26 | −0.05 | P | 3.705 | −4.404 | 1 | 0.94 ± 0.06 | 0.31 | |
105858 | 6089 | 4.38 | −0.68 | P | 1.400 | −4.491 | 1 | 2.93 ± 0.57 | 0.57 | |
109176 | 6448 | 4.25 | 0.12 | P | 3.303 | −5.06 | 7 | 4.61 ± 0.39 | 7.72 | |
113283 | 4555 | 4.53 | −0.01 | S | 0.181 | −4.467 | 1 | 16.03 ± 0.03 | 0.88 | 0.49 |
116771 | 6180 | 4.09 | −0.10 | S | 3.319 | −5.112 | 4 | >8.58 (6.67) | > 2.27 | |
FGK stars (15 pc <d ≤ 20 pc) | ||||||||||
|
||||||||||
5862 | 6128 | 4.36 | + 0.16 | S | 1.913 | −4.861 | 1 | 13.63 ± 0.68 | 2.17 | 4.12 |
17651 | 6654 | 4.11 | + 0.09 | P | 4.930 | −4.684 | 1 | 2.74 ± 0.40 | 1.83 | |
36366 | 7086 | 4.13 | −0.25 | P | 5.351 | −4.66 | 6 | 2.50 ± 0.36 ‡ | 1.61 | |
44248 | 6556 | 4.01 | + 0.04 | P | 5.249 | −4.548 | 8 | 2.62 ± 0.09 | 0.83 | |
46509 | 6486 | 4.22 | −0.01 | P | 3.369 | −4.828 | 4 | 2.66 ± 0.52 | 3.61 | |
48113 | 5940 | 4.05 | + 0.14 | S | 2.618 | −5.042 | 4 | 22.30 ± 0.89 | 3.91 | 7.39 |
61174 | 6784 | 4.06 | −0.05 | P | 4.873 | −5.173 | 6 | >1.12 (59.15) | ||
64241 | 6376 | 4.26 | −0.21 | P | 4.625 | −4.53 | 2 | 2.26 ± 0.20 | 0.74 | |
67153 | 6745 | 3.88 | −0.09 | P | 5.857 | −4.56 | 6 | 2.42 ± 0.22 ‡ | 0.90 | |
71284 | 6727 | 4.32 | −0.35 | S | 3.112 | −5.476 | 4 | >9.34 (7.32) | ||
75312 | 5949 | 4.15 | −0.06 | S | 2.631 | −4.828 | 2 | 13.60 ± 0.38 | 2.07 | 3.61 |
77760 | 5840 | 3.94 | −0.49 | S | 2.962 | −5.042 | 2 | 15.50 ± 1.59 | 2.91 | 7.39 |
88745 | 6089 | 4.18 | −0.53 | S | 1.867 | −5.02 | 9 | 11.52 ± 0.20 | 2.60 | 6.98 |
104858 | 6250 | 4.40 | −0.07 | P | 4.450 | −4.905 | 8 | 10.36 ± 1.32 | 2.12 | 4.86 |
112447 | 6181 | 3.93 | −0.24 | S | 4.387 | −5.276 | 4 | >4.55 (12.67) | > 1.23 |
Notes. Teff, log g, and [Fe/H] are averages from Fuhrmann (2008), Gray et al. (2003), Gray et al. (2006), Holmberg et al. (2009), Santos et al. (2004), Sousa et al. (2008), Takeda et al. (2005), and Valenti & Fischer (2005). “S” and “P” in Col. 5 mean that the determination is spectroscopic or photometric. log g for HIP 104858 assigned according to its spectral type.
Reference. : (1) Gray et al. (2006); (2) Baliunas et al. (1996); (3) Martínez-Arnáiz et al. (2010); (4) Duncan et al. (1991); (5) Hall et al. (2007); (6)
computed from ROSAT X-ray data using Eq. (A1) from Mamajek & Hillenbrand (2008); (7) Saffe et al. (2005); (8) Gray et al. (2003); (9) Wright et al. (2004). Determination of Prot from the Rossby number and
valid if 0.4 <B − V< 1.4 and
(Noyes et al. 1984).
When a lower limit of the period is given, the number in parentheses is the value of vsini (km s-1) used to estimate it.
The (B − V) value is slightly outside the valid range of the Noyes et al. (1984) calibration for Prot. Gyrochronology age calibration valid if B − V> 0.5 (Mamajek & Hillenbrand 2008). Chromospheric age calibration valid in the interval (Mamajek & Hillenbrand 2008).
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