Table 1.
Triangulum stream member stars.
No. | αJ2000 | δJ2000 | ![]() |
![]() |
μδ | σμδ | Vr | σVr | [Fe/H] | σ[Fe/H] | G | GBP | GRP | Survey |
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
(°) | (°) | (mas yr−1) | (mas yr−1) | (mas yr−1) | (mas yr−1) | (km s−1) | (km s−1) | (dex) | (dex) | (mag) | (mag) | (mag) | ||
1⋆ | 23.8285 | 22.8031 | 1.0098 | 0.0986 | −0.1037 | 0.0784 | −16.84 | 3.11 | −1.913 | 0.068 | 16.759 | 17.222 | 16.106 | SEGUE |
2⋆× | 24.1829 | 22.9364 | 1.0127 | 0.1831 | −0.9748 | 0.1339 | 2.78 | 7.84 | −2.545 | 0.048 | 17.617 | 18.049 | 16.997 | SEGUE |
3⋆ | 24.2157 | 22.9598 | 0.8790 | 0.3456 | 0.2562 | 0.2288 | −17.60 | 8.73 | −1.867 | 0.104 | 18.530 | 19.005 | 17.998 | SEGUE |
4⋆ (BHB) | 23.2433 | 23.1934 | 0.6858 | 0.1844 | −0.2179 | 0.1546 | −32.59 | 6.76 | −2.121 | 0.078 | 17.967 | 18.031 | 17.815 | SEGUE |
5⋆ | 24.1515 | 23.3639 | 1.2849 | 0.1128 | 0.2147 | 0.0938 | −23.76 | 4.55 | −2.348 | 0.114 | 17.335 | 17.803 | 16.718 | SEGUE |
6⋆ | 23.9200 | 23.3903 | 0.5511 | 0.2549 | 0.4586 | 0.1641 | −26.84 | 7.61 | −2.128 | 0.114 | 18.251 | 18.672 | 17.667 | SEGUE |
7⋆ | 23.8055 | 23.4783 | 1.1128 | 0.2314 | 0.0493 | 0.1889 | −16.15 | 8.19 | −2.371 | 0.056 | 18.457 | 18.891 | 17.927 | SEGUE |
8 (BHB) | 24.5968 | 23.6575 | 1.1237 | 0.1755 | 0.1393 | 0.1465 | −28.03 | 4.77 | −2.278 | 0.152 | 17.834 | 17.903 | 17.692 | SEGUE |
9⋆ | 23.7817 | 23.8800 | 1.0403 | 0.2248 | 0.2268 | 0.1843 | −36.43 | 5.51 | −2.383 | 0.095 | 18.256 | 18.669 | 17.716 | SEGUE |
10⋆ | 23.9193 | 24.1185 | 0.8721 | 0.2242 | −0.1813 | 0.1614 | −31.52 | 5.94 | −1.953 | 0.128 | 18.220 | 18.705 | 17.689 | SEGUE |
11 | 24.0593 | 24.1634 | 1.0918 | 0.0460 | 0.1548 | 0.0351 | −27.93 | 8.18 | −2.249 | 0.061 | 15.279 | 15.832 | 14.573 | LAMOST |
12⋆ | 23.4145 | 24.3451 | 1.5329 | 0.3380 | 0.0838 | 0.1762 | −22.60 | 9.99 | −2.072 | 0.072 | 18.648 | 18.981 | 18.075 | SEGUE |
13⋆ | 23.5792 | 24.3911 | 1.1712 | 0.2725 | 0.3187 | 0.1921 | −13.69 | 9.70 | −2.653 | 0.147 | 18.648 | 19.030 | 18.073 | SEGUE |
14 | 23.5445 | 24.5692 | 1.0955 | 0.0584 | 0.1400 | 0.0363 | −32.73 | 9.18 | −1.962 | 0.135 | 16.025 | 16.537 | 15.347 | LAMOST |
15 | 23.8850 | 24.7038 | 0.9478 | 0.1592 | 0.0680 | 0.1383 | −24.41 | 6.23 | −1.830 | 0.140 | 17.839 | 18.239 | 17.246 | SEGUE |
16 | 22.3385 | 28.4684 | 0.9975 | 0.0801 | 0.3481 | 0.0569 | −41.53 | 12.97 | −2.311 | 0.111 | 16.581 | 17.045 | 15.961 | LAMOST |
17 | 22.4622 | 30.0863 | 0.9254 | 0.1081 | 0.0873 | 0.0825 | −34.82 | 9.93 | −1.716 | 0.272 | 17.156 | 17.596 | 16.563 | LAMOST |
18 | 22.3181 | 31.2075 | 0.9126 | 0.0968 | 0.0614 | 0.0716 | −57.01 | 16.48 | −2.143 | 0.241 | 17.152 | 17.616 | 16.521 | LAMOST |
19 | 21.4457 | 34.2315 | 0.8154 | 0.0552 | 0.2357 | 0.0419 | −68.02 | 13.15 | −2.439 | 0.161 | 15.964 | 16.453 | 15.313 | LAMOST |
20 | 20.8085 | 34.9178 | 0.7522 | 0.0638 | 0.4043 | 0.0443 | −75.26 | 12.41 | −2.056 | 0.136 | 16.213 | 16.680 | 15.569 | LAMOST |
21 | 21.2461 | 35.1423 | 0.9246 | 0.1032 | 0.4356 | 0.0884 | −74.81 | 12.45 | −2.322 | 0.204 | 17.493 | 17.885 | 16.919 | LAMOST |
22 | 21.3470 | 35.2527 | 0.8679 | 0.0563 | 0.2653 | 0.0435 | −74.42 | 11.61 | −2.141 | 0.211 | 16.273 | 16.759 | 15.613 | LAMOST |
23 | 20.6703 | 37.3033 | 0.5967 | 0.2600 | 0.3732 | 0.2044 | −76.24 | 12.45 | −2.145 | 0.038 | 19.007 | 19.514 | 18.485 | SEGUE |
24 (BHB) | 20.4665 | 37.9600 | 0.7622 | 0.1674 | 0.3160 | 0.1455 | −90.22 | 5.21 | −1.740 | 0.055 | 18.101 | 18.157 | 18.010 | SEGUE |
25 | 20.6305 | 38.4133 | 0.9838 | 0.1966 | 0.2130 | 0.1741 | −87.51 | 7.20 | −2.042 | 0.089 | 18.524 | 18.966 | 17.931 | SEGUE |
26 (BHB) | 20.7368 | 38.4931 | 1.0037 | 0.1538 | 0.2964 | 0.1236 | −105.28 | 7.22 | −1.378 | 0.040 | 17.908 | 18.044 | 17.637 | SEGUE |
27 | 20.1517 | 38.6458 | 0.8931 | 0.1369 | 0.2047 | 0.0976 | −101.34 | 5.60 | −2.036 | 0.041 | 17.676 | 18.130 | 17.124 | SEGUE |
Notes. Identified member stars of Triangulum stream, sorted by δ. Common stars of Martin et al. (2013) are marked with “⋆.” An outlier identified in μδ panel of Fig. 3 is further labeled in “×.” Columns 12–14 are Gaia magnitudes that have been extinction-corrected (see text). The last column indicates which survey the radial velocity and metallicity come from.
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