Table 2
The RGB sample: fit results.
HIP | Teff | Dust | L | θ | τV | Ṁ | Code |
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|
(K) | ( L⊙) | (mas) | (M⊙ yr-1) | ||||||
|
|||||||||
4147 | 3800 | 1044 ± 25 | 3.85 ± 0.15 | 10-5 | 1.05 × 10-12 | 0 | 74 | ||
12 107 | 3700 | 482 ± 18 | 3.47 ± 0.15 | 10-5 | 4.88 × 10-13 | 0 | 278 | ||
32 173 | 3900 | 219 ± 09 | 3.03 ± 0.13 | 10-5 | 4.95 × 10-13 | 0 | 228 | ||
37 300 | 3800 | 665 ± 10 | 3.43 ± 0.13 | 10-5 | 8.41 × 10-13 | 0 | 13 | ||
37 946 | 3700 | 599 ± 15 | 4.15 ± 0.17 | 10-5 | 5.44 × 10-13 | 0 | 70 | ||
41 822 | 3900 | 259 ± 11 | 2.58 ± 0.11 | 10-5 | 5.38 × 10-13 | 0 | 189 | ||
44 126 | 3600 | iron | 528 ± 16 | 2.92 ± 0.12 | (4.99 ± 0.15) × 10-2 | 2.54 × 10-09 | 1 | 46 | |
44 390 | 3600 | iron | 522 ± 14 | 5.65 ± 0.23 | (8.36 ± 0.94) × 10-3 | 4.21 × 10-10 | 1 | 34 | |
44 857 | 3800 | 560 ± 20 | 3.17 ± 0.13 | 10-5 | 7.72 × 10-13 | 0 | 202 | ||
46 750 | 3800 | 467 ± 10 | 4.59 ± 0.18 | 10-5 | 7.05 × 10-13 | 0 | 60 | ||
47 723 | 3700 | 842 ± 24 | 3.51 ± 0.14 | 10-5 | 9.21 × 10-13 | 0 | 97 | ||
49 005 | 4000 | 293 ± 04 | 2.15 ± 0.08 | 10-5 | 5.85 × 10-13 | 0 | 8 | ||
49 029 | 3700 | iron | 688 ± 18 | 4.76 ± 0.19 | (8.04 ± 0.74) × 10-3 | 4.69 × 10-10 | 1 | 31 | |
52 366 | 3600 | iron | 1207 ± 32 | 3.33 ± 0.14 | (3.56 ± 0.15) × 10-2 | 2.73 × 10-09 | 1 | 28 | |
52 863 | 3700 | 384 ± 13 | 2.65 ± 0.11 | 10-5 | 6.22 × 10-13 | 0 | 82 | ||
53 449 | 3300 | iron | 1346 ± 44 | 8.77 ± 0.40 | (5.58 ± 0.20) × 10-2 | 4.41 × 10-09 | 1 | 41 | |
53 726 | 3600 | 1071 ± 32 | 3.09 ± 0.13 | 10-5 | 7.20 × 10-13 | 0 | 99 | ||
53 907 | 3800 | 1095 ± 34 | 3.95 ± 0.16 | 10-5 | 1.08 × 10-12 | 0 | 107 | ||
54 537 | 3700 | 410 ± 16 | 2.73 ± 0.12 | 10-5 | 6.43 × 10-13 | 0 | 178 | ||
55 687 | 3900 | iron | 353 ± 08 | 3.31 ± 0.12 | (5.62 ± 5.16) × 10-4 | 2.39 × 10-11 | 1 | 30 | |
56 127 | 3900 | iron | 975 ± 55 | 3.41 ± 0.16 | (8.08 ± 0.51) × 10-3 | 5.72 × 10-10 | 1 | 177 | |
56 211 | 3700 | 959 ± 16 | 6.85 ± 0.27 | 10-5 | 9.83 × 10-13 | 0 | 32 | ||
60 122 | 3700 | 836 ± 20 | 3.60 ± 0.14 | 10-5 | 6.43 × 10-13 | 0 | 61 | ||
60 795 | 3800 | 246 ± 06 | 2.62 ± 0.10 | 10-5 | 5.12 × 10-13 | 0 | 69 | ||
61 658 | 3600 | iron | 601 ± 22 | 3.88 ± 0.17 | (1.94 ± 0.088) × 10-2 | 1.05 × 10-09 | 1 | 70 | |
62 443 | 3700 | 279 ± 14 | 2.11 ± 0.10 | 10-5 | 5.31 × 10-13 | 0 | 363 | ||
63 355 | 3800 | iron | 324 ± 12 | 3.88 ± 0.16 | (4.14 ± 0.70) × 10-3 | 1.67 × 10-10 | 1 | 50 | |
64 607 | 3900 | iron | 267 ± 13 | 2.26 ± 0.10 | (1.28 ± 0.061) × 10-2 | 4.75 × 10-10 | 1 | 129 | |
66 417 | 3700 | 336 ± 07 | 2.95 ± 0.12 | 10-5 | 5.82 × 10-13 | 0 | 46 | ||
66 738 | 3600 | 1458 ± 32 | 5.67 ± 0.23 | 10-5 | 8.40 × 10-13 | 0 | 55 | ||
67 605 | 3800 | iron | 545 ± 13 | 2.40 ± 0.09 | (1.47 ± 0.13) × 10-2 | 7.72 × 10-10 | 1 | 26 | |
67 627 | 3500 | 1113 ± 19 | 7.40 ± 0.30 | 10-5 | 7.26 × 10-13 | 0 | 31 | ||
67 665 | 3600 | iron | 1895 ± 73 | 5.64 ± 0.24 | (3.96 ± 0.096) × 10-2 | 3.81 × 10-09 | 1 | 61 | |
69 068 | 3700 | iron | 790 ± 23 | 3.78 ± 0.15 | (1.66 ± 0.059) × 10-2 | 1.04 × 10-09 | 1 | 61 | |
69 373 | 3700 | iron | 477 ± 17 | 3.76 ± 0.16 | (5.18 ± 0.63) × 10-3 | 2.52 × 10-10 | 1 | 68 | |
71 280 | 3900 | iron | 818 ± 76 | 2.22 ± 0.13 | (1.45 ± 0.065) × 10-2 | 9.42 × 10-10 | 1 | 426 | |
73 568 | 4000 | 318 ± 09 | 3.02 ± 0.11 | 10-5 | 6.09 × 10-13 | 0 | 101 | ||
76 307 | 3800 | iron | 937 ± 36 | 3.45 ± 0.14 | (2.60 ± 0.71) × 10-3 | 1.79 × 10-10 | 1 | 80 | |
77 661 | 3900 | AlOx | 358 ± 06 | 3.35 ± 0.12 | (5.00 ± 1.59) × 10-4 | 3.16 × 10-11 | 1 | 24 | |
78 632 | 3800 | 844 ± 18 | 2.11 ± 0.08 | 10-5 | 9.45 × 10-13 | 0 | 29 | ||
80 042 | 3900 | iron | 302 ± 07 | 1.52 ± 0.06 | (6.69 ± 0.17) × 10-2 | 2.66 × 10-09 | 1 | 30 | |
80 197 | 3700 | iron | 1157 ± 32 | 3.90 ± 0.16 | (1.50 ± 0.064) × 10-2 | 1.14 × 10-09 | 1 | 47 | |
80 214 | 4000 | 426 ± 22 | 2.19 ± 0.10 | 10-5 | 7.06 × 10-13 | 0 | 305 | ||
82 073 | 3900 | 224 ± 05 | 2.80 ± 0.11 | 10-5 | 5.01 × 10-13 | 0 | 63 | ||
83 430 | 3700 | iron | 526 ± 10 | 4.28 ± 0.17 | (1.71 ± 0.11) × 10-2 | 8.74 × 10-10 | 1 | 23 | |
84 835 | 3800 | 455 ± 15 | 2.67 ± 0.11 | 10-5 | 6.96 × 10-13 | 0 | 157 | ||
87 833 | 3900 | 602 ± 04 | 10.55 ± 0.38 | 10-5 | 8.20 × 10-13 | 0 | 4 | ||
88 122 | 4000 | iron | 351 ± 15 | 2.07 ± 0.08 | (4.11 ± 0.084) × 10-2 | 1.77 × 10-09 | 1 | 60 | |
98 401 | 3700 | iron | 285 ± 13 | 2.37 ± 0.10 | (5.59 ± 0.67) × 10-3 | 2.10 × 10-10 | 1 | 121 | |
106 140 | 3700 | 682 ± 12 | 4.89 ± 0.19 | 10-5 | 8.29 × 10-13 | 0 | 33 | ||
112 716 | 3900 | 567 ± 13 | 4.98 ± 0.19 | 10-5 | 7.96 × 10-13 | 0 | 54 | ||
114 144 | 3900 | iron | 373 ± 08 | 3.90 ± 0.15 | (7.07 ± 8.43) × 10-4 | 3.10 × 10-11 | 1 | 34 | |
115 669 | 4000 | 262 ± 04 | 3.60 ± 0.13 | 10-5 | 3.70 × 10-13 | 0 | 10 | ||
117 718 | 3600 | 816 ± 19 | 4.82 ± 0.20 | 10-5 | 6.29 × 10-13 | 0 | 68 |
Notes. Listed are, (Col. 2) the effective temperature of the MARCS model, (Col. 3) the dust component that fits best in the case when τV ≠ 10-5, (Col. 4) luminosity and the internal error (that is, the error in the Hipparcos distance is not included), (Col. 5) the angular diameter in mas and the error (based on the error in L, and a 70 K error in Teff), (Col. 6) the dust optical depth in the V-band and the internal error, and (Col. 7) the corresponding mass-loss rate assuming a constant expansion velocity of 10 km s-1, a dust-to-gas (Ψ) ratio of 0.005 and grain specific density, ρ, of 5.1 g cm-3 (appropriate for iron grains in a DHS with 70% vacuum), (Col. 8) a code if the optical depth was fitted (1) or fixed (0), (Col. 9) the reduced χ2 to indicate the goodness of the fit.
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