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Table E.17.

Stellar properties for the Hyades LDB sample. Quantities obtained from Hogan et al. (2008).

Object ϖ μαcos(δ) μδ ρμα *  μδ dMAP dmin dmax Teffχ2 Lbol −ΔLbol Lbol
[mas] [mas yr−1] [mas yr−1] [pc] [pc] [pc] [K] [10−3L] [10−3L] [10−3L]
Hya03 - - 102.46 - -7.86 - - 54.60 50.88 58.32 2 298 0.217 0.160 0.285
Hya08 - - 82.99 - -19.34 - - 44.80 41.12 48.48 1 993 0.171 0.106 0.254
Hya11 - - 165.09 - -32.33 - - 37.60 36.04 39.16 1 512 0.083 0.071 0.095
Hya09 - - 72.04 - -22.32 - - 57.80 52.44 63.16 2 000 0.174 0.142 0.209
Hya10 - - 108.27 - -29.45 - - 47.80 44.82 50.78 1 771 0.084 0.069 0.101
Hya12 - - 112.04 - -17.86 - - 41.40 38.84 43.96 1 811 0.061 0.045 0.080

Hya01 - - 148.98 - -46.41 - - 36.20 34.57 37.83 2 384 0.247 0.220 0.276
Hya06 - - 99.37 - -23.48 - - 50.90 47.41 54.39 2 324 0.206 0.170 0.247
Hya05 - - 125.14 - -24.32 - - 46.60 44.04 49.16 2 000 0.189 -0.058 0.496
Hya02 - - 114.31 - -36.95 - - 52.80 49.72 55.88 1 970 0.216 0.181 0.255
Hya04 - - 82.71 - -21.25 - - 54.40 49.94 58.86 1 986 0.219 0.180 0.263
Hya07 - - 86.98 - -28.14 - - 53.00 48.94 57.06 1 535 0.196 0.165 0.229

Note: The distances and proper motions were taken from Hogan et al. (2008). Bolometric luminosities were calculated using these distances.

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