Table A.1.
Properties of the 137 cluster members selected from our membership analysis in Lupus.
Source Identifier | α | δ | μα cos δ | μδ | ϖ | RUWE | Prob. | Vr | Ref | d | U | V | W | Cloud | α | SED |
---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
(h:m:s) | (° ′ ′ < SPSDOUBLEDOLLAR > ′) | (mas yr−1) | (mas yr−1) | (mas) | (km s−1) | (pc) | (km s−1) | (km s−1) | (km s−1) | |||||||
Gaia DR2 6013399894569703040 | 15 39 27.76 | -34 46 17.6 | −13.271 ± 0.120 | −22.242 ± 0.069 | 6.439 ± 0.052 | 1.02 | 0.9307 | −2.7 ± 2.0 | 1 |
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Lupus 1 | −1.22 ± 0.14 | Class II |
Gaia DR2 6013073790593533824 | 15 44 00.94 | -35 31 06.1 | −11.492 ± 0.264 | −24.071 ± 0.187 | 6.454 ± 0.140 | 1.22 | 0.9701 |
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Lupus 1 | −2.47 ± 0.11 | Class III | |||||
Gaia DR2 6014696841553696768 | 15 45 12.85 | -34 17 31.0 | −13.625 ± 0.128 | −21.605 ± 0.081 | 6.485 ± 0.060 | 1.83 | 0.8220 |
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Lupus 1 | |||||||
Gaia DR2 6014769134444800896 | 15 46 42.97 | -34 30 11.9 | −12.575 ± 0.395 | −22.158 ± 0.258 | 6.088 ± 0.214 | 2.92 | 0.8569 |
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Lupus 1 | |||||||
Gaia DR2 6007849461103723136 | 15 47 11.58 | -41 01 18.5 | −13.475 ± 0.167 | −22.863 ± 0.115 | 6.405 ± 0.082 | 2.05 | 0.8716 |
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off-cloud | |||||||
Gaia DR2 6011581856393988352 | 15 48 06.24 | -35 15 48.5 | −12.124 ± 0.195 | −22.325 ± 0.129 | 6.607 ± 0.093 | 1.31 | 0.9461 |
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Lupus 1 | |||||||
Gaia DR2 6011500389453302272 | 15 49 30.72 | -35 49 51.8 | −12.767 ± 0.110 | −23.370 ± 0.077 | 6.268 ± 0.051 | 1.07 | 0.9620 | 1.4 ± 1.0 | 1 |
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Lupus 1 | −1.37 ± 0.27 | Class II |
Gaia DR2 5995437246144906496 | 15 51 31.67 | -43 02 04.8 | −8.830 ± 0.977 | −22.605 ± 0.671 | 5.577 ± 0.487 | 10.94 | 0.8366 |
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off-cloud | |||||||
Gaia DR2 6011392186336443392 | 15 51 46.94 | -35 56 44.5 | −12.418 ± 0.088 | −24.158 ± 0.058 | 6.459 ± 0.052 | 1.15 | 0.9602 | −2.6 ± 0.1 | 2 |
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off-cloud | −1.24 ± 0.28 | Class II |
Gaia DR2 6011827867821601792 | 15 55 10.26 | -34 55 05.0 | −11.096 ± 0.535 | −23.941 ± 0.306 | 6.778 ± 0.257 | 0.96 | 0.9191 |
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off-cloud | −1.12 ± 0.13 | Class II | |||||
Gaia DR2 6010133559067032832 | 15 55 50.27 | -38 01 34.1 | −11.659 ± 0.129 | −22.951 ± 0.078 | 6.255 ± 0.061 | 1.18 | 0.9961 | −0.1 ± 2.9 | 1 |
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Lupus 2 | ||
Gaia DR2 6010133559067032704 | 15 55 50.32 | -38 01 32.2 | −11.787 ± 0.173 | −23.359 ± 0.103 | 6.249 ± 0.080 | 2.70 | 0.9034 |
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Lupus 2 | |||||||
Gaia DR2 6010483616079976448 | 15 56 02.08 | -36 55 28.6 | −11.660 ± 0.073 | −22.503 ± 0.047 | 6.329 ± 0.037 | 1.03 | 0.9918 | 2.6 ± 1.2 | 1 |
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off-cloud | −1.20 ± 0.14 | Class II |
Gaia DR2 6010135758090335232 | 15 56 09.19 | -37 56 06.5 | −12.091 ± 0.120 | −23.718 ± 0.074 | 6.311 ± 0.054 | 1.27 | 0.9957 | −1.0 ± 1.0 | 3 |
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Lupus 2 | −1.02 ± 0.13 | Class II |
Gaia DR2 5994793310284482432 | 15 56 37.72 | -42 42 45.0 | −10.443 ± 0.369 | −22.872 ± 0.249 | 5.986 ± 0.175 | 1.01 | 0.8959 |
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Lupus 4 | −2.48 ± 0.12 | Class III | |||||
Gaia DR2 5994795990344219904 | 15 56 38.11 | -42 35 57.6 | −12.117 ± 0.304 | −23.561 ± 0.212 | 6.420 ± 0.145 | 1.04 | 0.9352 |
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Lupus 4 | −2.26 ± 0.05 | Class III | |||||
Gaia DR2 6010114558131195392 | 15 56 42.30 | -37 49 15.8 | −11.546 ± 0.139 | −23.234 ± 0.090 | 6.267 ± 0.067 | 1.80 | 0.9966 |
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Lupus 2 | |||||||
Gaia DR2 5994793241564999040 | 15 56 44.20 | -42 42 24.9 | −10.973 ± 0.197 | −22.833 ± 0.133 | 6.140 ± 0.097 | 1.13 | 0.9709 |
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Lupus 4 | |||||||
Gaia DR2 5994747367001754240 | 15 57 23.99 | -42 40 04.9 | −11.259 ± 0.075 | −23.205 ± 0.052 | 6.229 ± 0.035 | 0.98 | 0.9962 |
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Lupus 4 | −1.10 ± 0.14 | Class II | |||||
Gaia DR2 5994831449595857408 | 15 57 30.32 | -42 10 32.8 | −11.671 ± 0.109 | −23.292 ± 0.076 | 6.204 ± 0.052 | 1.42 | 0.9931 |
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Lupus 4 |
Notes. This table is available in CDS.
For each star, we provide the Gaia-DR2 identifier, position, proper motion and parallax (not corrected for zero-point offset) from the Gaia-DR2 catalogue, RUWE, membership probability, radial velocity with reference, distance derived from Bayesian inference, UVW spatial velocity, molecular cloud, spectral index, and object class based on the SED. References for radial velocities: (1) Frasca et al. (2017), (2) Guenther et al. (2007), (3) Wichmann et al. (1999), (4) Gontcharov (2006), and (5) Galli et al. (2013).
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