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Table 4.

Physical parameters of BHB and post-EHB candidates computed adopting the atmospheric parameters derived from metal deficient atmospheric models and a mass of M = 0.5 ± 0.1 M.

Short name R/R log L/L D(SpT)
(kpc)
0035−5900
0038−6612
0039−4201
0049−5356
0122−6759
0245−3418
1715+2341
1839−7515
1851−5036
1900−7032
1919−5938
2019−7107
2024−2725
2028−2218
2110−2700
2114−6438
2119−4827
2125−4834
2145−3022
2207−5021
2208−6026
2213−4357
2214−4620
2239−2455
2250−5625
2313−4858
2348−6612

1621−8350 (a)
1944−4628 (a) 2.46
1944−4628B (a) 1.34 −0.06

Notes. The two hot post-EHB stars are listed at the end. 1944−4628B denotes the cool companion of 1944−4628.

(a)

Based on solar-metallicity models.

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