Table 10: The cross-identification of known multiple star systems and their astrometric segregation from this work (last column). First column is our identification number (Table 3), second column that from BDA and third that from Sanders (1977).
ID$_{\rm 3}$ ID $_{\rm BDA}$ ID$_{\rm S}$ b-y V m1 c1 $H_{\beta}$ M/NM
609 22 821 0.371$\pm$0.001 12.764$\pm$0.003 0.150$\pm$0.002 0.436$\pm$0.003   M
629 24 760 0.375$\pm$0.001 13.307$\pm$0.003 0.180$\pm$0.002 0.418$\pm$0.004 2.683$\pm$0.041 M
761 55 752 0.181$\pm$0.001 11.310$\pm$0.003 0.230$\pm$0.002 0.841$\pm$0.004 2.735$\pm$0.006 M
777 61 757 0.425$\pm$0.004 13.530$\pm$0.003 0.124$\pm$0.006 0.410$\pm$0.008 2.640$\pm$0.000 M
806 65 1077 0.435$\pm$0.002 12.587$\pm$0.003 0.173$\pm$0.003 0.358$\pm$0.004 2.638$\pm$0.005  
905 86 1063 0.630$\pm$0.001 13.538$\pm$0.003 0.377$\pm$0.002 0.244$\pm$0.004 2.575$\pm$0.008 M
910 88 1053 0.417$\pm$0.001 12.245$\pm$0.003 0.211$\pm$0.002 0.375$\pm$0.004 2.605$\pm$0.008 M
924 90 975 0.281$\pm$0.001 11.063$\pm$0.003 0.166$\pm$0.002 0.676$\pm$0.004 2.666$\pm$0.011 NM
962 102 2206 0.463$\pm$0.001 12.396$\pm$0.003 0.241$\pm$0.002 0.346$\pm$0.004 2.607$\pm$0.014 M
992 111 986 0.366$\pm$0.001 12.725$\pm$0.003 0.177$\pm$0.002 0.414$\pm$0.003 2.624$\pm$0.010 M
1005 117 999 0.491$\pm$0.001 12.569$\pm$0.003 0.254$\pm$0.002 0.308$\pm$0.003 2.595$\pm$0.003 M
1015 119 1045 0.384$\pm$0.001 12.539$\pm$0.003 0.165$\pm$0.002 0.393$\pm$0.003 2.621$\pm$0.004 M
1029 123 1070 0.403$\pm$0.004 13.985$\pm$0.003 0.167$\pm$0.004 0.343$\pm$0.005 2.601$\pm$0.012 M
1033 124 997 0.292$\pm$0.001 12.143$\pm$0.003 0.172$\pm$0.002 0.536$\pm$0.004 2.646$\pm$0.005 M
1046 131 1082 0.266$\pm$0.003 11.260$\pm$0.003 0.120$\pm$0.006 0.731$\pm$0.008 2.704$\pm$0.007 M
1050 134 984 0.367$\pm$0.001 12.259$\pm$0.003 0.180$\pm$0.002 0.409$\pm$0.004 2.626$\pm$0.000 M
1060 136 1072 0.418$\pm$0.001 11.279$\pm$0.003 0.160$\pm$0.002 0.452$\pm$0.004 2.629$\pm$0.007 M
1101 143 1040 0.545$\pm$0.001 11.466$\pm$0.003 0.319$\pm$0.002 0.330$\pm$0.003 2.531$\pm$0.037 M
1102 144 1000 0.484$\pm$0.001 12.836$\pm$0.003 0.253$\pm$0.002 0.364$\pm$0.004 2.596$\pm$0.002 NM
1176 161 1036 0.327$\pm$0.004 12.760$\pm$0.004 0.159$\pm$0.005 0.380$\pm$0.008 2.660$\pm$0.006 M
1206 170 1250 0.823$\pm$0.012 9.769$\pm$0.009 0.555$\pm$0.012 0.372$\pm$0.009 2.593$\pm$0.009 M
1223 173 1264 0.608$\pm$0.001 12.063$\pm$0.003 0.428$\pm$0.002 0.337$\pm$0.004 2.589$\pm$0.012 NM
1237 176 1234 0.353$\pm$0.002 12.627$\pm$0.003 0.165$\pm$0.021 0.393$\pm$0.046 2.626$\pm$0.008 M
1300 190 1284 0.166$\pm$0.002 10.912$\pm$0.003 0.173$\pm$0.003 0.908$\pm$0.004 2.776$\pm$0.003 M
1324 195 1242 0.436$\pm$0.002 12.684$\pm$0.003 0.197$\pm$0.003 0.362$\pm$0.004 2.632$\pm$0.025 M
1352 205 1282 0.644$\pm$0.028 13.334$\pm$0.010 -0.086$\pm$0.030 0.350$\pm$0.028 2.460$\pm$0.028 M
1351 207 1195 0.264$\pm$0.001 12.301$\pm$0.003 0.143$\pm$0.003 0.551$\pm$0.004   M
1402 216 1216 0.387$\pm$0.004 12.673$\pm$0.004 0.136$\pm$0.004 0.379$\pm$0.004 2.728$\pm$0.056 M
1412 219 1272 0.385$\pm$0.001 12.530$\pm$0.003 0.163$\pm$0.002 0.380$\pm$0.004 2.679$\pm$0.075 M
1428 224 1221 0.696$\pm$0.001 10.730$\pm$0.003 0.517$\pm$0.003 0.308$\pm$0.004 2.713$\pm$0.005 M
1488 244 1237 0.583$\pm$0.002 10.741$\pm$0.003 0.350$\pm$0.003 0.350$\pm$0.005   M
987 1050 972 0.556$\pm$0.003 15.395$\pm$0.004 0.277$\pm$0.004 0.238$\pm$0.007 2.593$\pm$0.004  
1150 3079 - 0.668$\pm$0.003 15.788$\pm$0.003 0.430$\pm$0.005 0.139$\pm$0.008    
1567 3116 1508 0.364$\pm$0.005 12.823$\pm$0.004 0.185$\pm$0.006 0.386$\pm$0.007   M
1085 4004 1024 0.362$\pm$0.001 12.706$\pm$0.003 0.170$\pm$0.002 0.373$\pm$0.003 2.624$\pm$0.001 M
1126 5808 1113 0.621$\pm$0.001 13.703$\pm$0.003 0.321$\pm$0.003 0.188$\pm$0.006   M
1095 5748 1019 0.513$\pm$0.001 14.338$\pm$0.003 0.283$\pm$0.002 0.241$\pm$0.004 2.572$\pm$0.015 M
277 7440 440 0.800$\pm$0.002 8.992$\pm$0.003 -0.062$\pm$0.003 0.688$\pm$0.004   NM
524 32 723 0.535$\pm$0.001 15.690$\pm$0.003 0.366$\pm$0.004 0.341$\pm$0.006   M
1670 2134 1601 0.574$\pm$0.009 14.482$\pm$0.007 0.290$\pm$0.011 0.256$\pm$0.015   NM


Source LaTeX | All tables | In the text