Table 12

Table to replace Table 4 of Theissen et al. (1993). Deconvolved photometry, atmospheric parameters, and distances of the binary stars.

Object y by ub c1 T eff log g r z A y
(mag) (mag) (mag) (mag) (K) (cm s-2) (pc) (pc) (mag)

PG1647+253 14.179(095) 0.131(40) 0.272(47) 0.251(30) 36 500±1500 6.00 690 420 0.144
PG1701+359 13.250(089) 0.124(29) 0.095(44) 0.123(28) 26 250±1250 5.80 480 290 0.048
PG1718+519 14.284(019): 0.087(23): +0.037(10): 0.294(10): 23 500±1000: 4.25: 4120: 2370: 0.048
PG2110+127 13.230(011): 0.082(10): 0.045(06): 0.297(04): 25 400±1600: 4.20: 2670: 1070: 0.240
PG2259+134 14.635(146) 0.118(42) 0.138(79) 0.154(55) 28 500±1600 5.30 1650 1090 0.144
PG2331+038 15.090(150) 0.114(42) 0.102(80) 0.063(53) 27 200±1500 5.30 1940 1570 0.144
PG2337+070 13.613(132) 0.112(41) 0.090(67) 0.064(40) 27 250±1350 5.30 950 750 0.240
PHL1079 13.601(167) 0.110(43) 0.085(73) 0.217(60) 26 350±1450 5.10 1270 1070 0.048

Notes.

(∗)

Also discussed in Paper II (Moehler et al. 1990).

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