Open Access
Table A.3.
Eddington factors (Γe) and SED-fit parameters for the sample BSGs.
Star | Γe | DGaia [pc] | log C | log (L/L⊙) | MG [mag] |
HD 51309 | 0.18 | 1108![]() |
-1.49 | 4.84![]() |
-6.06![]() |
HD 64760 | 0.19 | 659![]() |
-1.67 | 4.91![]() |
-5.17![]() |
HD 74371 | 0.31 | 1718![]() |
-1.43 | 5.07![]() |
-6.87![]() |
HD 75149 | 0.31 | 1466![]() |
-1.47 | 5.16![]() |
-6.58![]() |
HD 77581 | 0.47 | 1969![]() |
-1.79 | 5.66![]() |
-6.51![]() |
HD 79186 | 0.39 | 1677![]() |
-1.41 | 5.29![]() |
-7.14![]() |
HD 80558 | 0.43 | 1862![]() |
-1.34 | 5.27![]() |
-7.27![]() |
HD 83183 | 0.12 | 593![]() |
-1.38 | 4.44![]() |
-5.16![]() |
HD 91619 | 0.44 | 2319![]() |
-1.48 | 5.18![]() |
-7.10![]() |
HD 92964 | 0.45 | 2130![]() |
-1.44 | 5.50![]() |
-7.46![]() |
HD 93840 | 0.26 | 2649![]() |
-2.22 | 4.64![]() |
-4.82![]() |
HD 94493 | 0.26 | 2167![]() |
-2.13 | 4.85![]() |
-5.11![]() |
HD 96248 | 0.44 | 2426![]() |
-1.81 | 5.27![]() |
-6.43![]() |
HD 99857 | 0.18 | 1794![]() |
-2.08 | 4.63![]() |
-4.75![]() |
HD 99953 | 0.43 | 2490![]() |
-1.64 | 5.37![]() |
-6.90![]() |
HD 103779 | 0.30 | 2039![]() |
-2.13 | 4.90![]() |
-5.05![]() |
HD 105071 | 0.24 | 2187![]() |
-1.62 | 4.73![]() |
-6.24![]() |
HD 106343 | 0.39 | 2379![]() |
-1.81 | 5.30![]() |
-6.51![]() |
HD 108002 | 0.32 | 2391![]() |
-1.93 | 5.07![]() |
-5.88![]() |
HD 109867 | 0.33 | 2552![]() |
-1.86 | 5.43![]() |
-6.56![]() |
HD 111558 | 0.16 | 4594![]() |
-1.86 | 4.90![]() |
-6.69![]() |
HD 111973 | 0.25 | 1948![]() |
-1.6 | 5.15![]() |
-6.57![]() |
HD 115842 | 0.51 | 1682![]() |
-1.71 | 5.57![]() |
-6.53![]() |
HD 116084 | 0.29 | 1958![]() |
-1.67 | 5.04![]() |
-6.36![]() |
HD 117024 | 0.16 | 1984![]() |
-1.98 | 4.47![]() |
-4.96![]() |
HD 119646 | 0.23 | 1721![]() |
-1.84 | 4.73![]() |
-5.40![]() |
HD 122879 | 0.52 | 2274![]() |
-1.91 | 5.59![]() |
-6.44![]() |
HD 125288 | 0.08 | 438![]() |
-1.34 | 4.13![]() |
-4.50![]() |
HD 125545 | 0.25 | 2171![]() |
-2.01 | 4.87![]() |
-5.29![]() |
HD 141318 | 0.11 | 596![]() |
-1.73 | 4.09![]() |
-3.71![]() |
HD 142758 | 0.38 | 3156![]() |
-1.86 | 5.19![]() |
-6.49![]() |
HD 148379 | 0.63 | 1585![]() |
-1.29 | 5.70![]() |
-7.66![]() |
HD 148688 | 0.49 | 1348![]() |
-1.44 | 5.60![]() |
-6.97![]() |
HD 149038 | 0.40 | 896![]() |
-1.67 | 5.33![]() |
-5.75![]() |
HD 150168 | 0.20 | 1015![]() |
-1.8 | 4.94![]() |
-5.54![]() |
HD 150898 | 0.29 | 1118![]() |
-1.87 | 4.99![]() |
-5.22![]() |
HD 152234 | 0.42 | 1935![]() |
-1.65 | 5.86![]() |
-7.16![]() |
HD 152235 | 0.40 | 1618![]() |
-1.6 | 5.55![]() |
-6.73![]() |
HD 154090 | 0.37 | 1116![]() |
-1.45 | 5.54![]() |
-6.76![]() |
HD 155985 | 0.25 | 1077![]() |
-1.83 | 4.82![]() |
-4.96![]() |
HD 157038 | 0.46 | 2168![]() |
-1.34 | 5.74![]() |
-7.89![]() |
Notes. The last two columns contain luminosities and the absolute G−band magnitudes, which were calculated using the distance values from Gaia (third column).
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