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Table 2

Members of Chamaeleon I included in the TGAS catalog.

Name Ra (ICRS) Dec (ICRS) V t Bt SpT Ref.
TYC 9414-33-1 161.657371 –77.601034 9.42 10.14 F0V 1
               
TYC 9414-186-1 164.778625 –77.027854 11.79 13.28 K4Ve 4
               
TYC 9410-1954-1 166.490488 –76.130243 7.70 7.87 B6IV/V 1
               
TYC 9414-787-1 166.563573 –77.365761 11.20 13.09 G5Ve 4 ...
               
HIP 54365 166.835926 –77.635358 11.02 11.84 G2Ve 2
               
TYC 9414-795-1 167.013356 –77.654853 8.49 8.85 A0Vep 4
               
TYC 9410-2805-1 167.458029 –76.613256 9.08 9.48 B9V 1
               
TYC 9410-60-1 168.115046 –76.739532 11.21 12.24 G9Ve 2
π [mas] σπ [mas] μα [mas/yr] [mas/yr] μδ [mas/yr] [mas/yr] E(BV ) d [pc] + 2σd − 2σd
4.84 0.21 –28.65 0.15 –9.02 0.13 0.927 0.291 207 +17 –13
                       
5.32 0.22 –22.76 0.26 2.21 0.24 0.164 0.393 188 +15 –11
                       
6.21 0.28 –22.35 0.04 0.69 0.03 0.411 0.139 162 +14 –11
                       
... 5.72 0.78 –27.08 3.83 6.04 1.75 0.318 0.144 178 +68 –29
                       
5.06 0.22 –22.51 0.20 1.30 0.17 0.093 0.199 198 +16 –13
                       
5.59 0.26 –22.46 0.05 1.25 0.05 0.309 0.159 179 +16 –12
                       
5.43 0.23 –21.43 0.10 –0.28 0.09 0.050 0.181 185 +15 –11
                       
5.03 0.22 –21.69 0.33 –0.86 0.29 0.260 0.079 199 +17 –13

References. Spectral type reference : (1) Houk & Cowley (1975); (2) Appenzeller (1977); (3) Irvine & Houk (1977); (4) Torres et al. (2006). V t and Bt are taken from H∅g et al. (2000). Proper motions are taken from TGAS (Gaia Collaboration 2016a). Distances are taken from Astraatmadja & Bailer-Jones (2016) computed with TGAS parallaxes assuming a Milky Way prior. The assumed distance is the mode of the posteriors and the quoted 2σ uncertainties the difference between this value and the 5 and 95 percentile values, respectively.

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