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Home All issues Volume 507 / No 2 (November IV 2009) A&A, 507 2 (2009) 1141-1201 Full HTML
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Table A.1:

OB eclipsing binaries of the HIPPARCOS catalog.
Var. HD HIP Var. Var. HIP New   CK $\langle H_{\rm p}\rangle $ Ampl. Sp.
name $N_{\rm o}$. $N_{\rm o}$. flag type P(d) P(d)   P(d) (mag) (mag) type
          OBMS   Total : 94        
V444 Cyg 193576 100214 P EA 4.213       8.060 0.243 O6
NX Vel 73882 42433 P E: 1.460       7.292 0.074 O8V:
V1182 Aql 175514 92865 P EB 1.622       8.747 0.191 O8:Vnn
TU Mus 100213 56196 P EB/KE 1.387       8.427 0.518 O8 (+O8)
V382 Cyg 228854 100135 P EB 1.886       8.730 0.830 O8
del Cir 135240 74778 P EA 3.902       5.056 0.154 O8.5V
AO Cas 1337 1415 P EB 3.523       6.062 0.198 O9IIInn
CC Cas 19820 15063 P EB/DM 3.366       7.237 0.108 O9IV
LZ Cep 209481 108772 P EB 3.070       5.554 0.099 O9V
LY Aur 35921 25733 P EB/SD 4.003       6.944 0.722 O9.5III
XZ Cep   111257 P EB/DM: 5.098       8.619 0.753 O9.5V
V745 Cas 1810 1805 P EW 1.411       8.104 0.142 B0IV
AB Cru 106871 59935 P EB 3.413       8.527 0.567 B0IVvar
V2107 Cyg 191473 99246 P EA 4.285       8.601 0.130 B0IV
Y Cyg 198846 102999 P EA/DM 2.996       7.335 0.473 B0IVv SB
NY Cep 217312 113461 P EA 15.276       7.514 0.086 B0IV
V478 Cyg 193611 100227 P EB 2.881       8.799 0.261 B0Vp
V649 Cas 219634 114904 P EA 2.391       6.598 0.069 B0Vn
UU Cas   117576 P EB/DM 8.520       9.934 0.379 B0.5III
del Pic 42933 29276 P EB/D: 1.673       4.651 0.205 B0.5IV
AI Cep 239767 107500 P EB/DM 4.225       9.424 0.577 B0.5V:pvar
  213405 110998a U EA?   2.847   2.847 8.099 0.077 B0.5V
AH Cep 216014 112562 P EW 1.775       6.977 0.277 B0.5V:nn
V431 Pup 69882 40596 P E 9.363       7.234 0.080 B1III:
VZ Cen 103146 57895 P EB 4.929       8.350 0.352 B1III:var
HX Lup 125721 70270 P EB? 3.088       6.056 0.046 B1III
V380 Cyg 187879 97634 P EA 12.426       5.676 0.101 B1III
V1898 Cyg 200776 103968 P EB 1.513       7.812 0.241 B1IV:p
EM Cep 208392 108073 P EW 0.806       7.085 0.126 B1IV:
eta Ori 35411 25281 P EA/BCE 7.990       3.312 0.243 B1V+B2
VV Ori 36695 26063 P EB 1.485       5.327 0.257 B1V
V Pup 65818 38957 P EB/SD 1.455       4.433 0.533 B1Vp+B2
LN Mus 110946 62339 P EB 3.672       9.265 0.311 B1V:
alf Vir 116658 65474 P EB? 4.014       0.888 0.035 B1V
eta Cen 127972 71352 P EB 1.285       2.276 0.071 B1Vn+A
pi. Sco 143018 78265 P EB 1.570       2.829 0.037 B1V+B2V
V1012 Sco 155775 84409 P EB 1.515       6.717 0.061 B1V
V701 Sco 317844 85985 P EW/KE 0.762       8.811 0.454 B1:V:nn
V1331 Aql 173198 91910d P EA 1.364       7.870 0.259 B1Vvar
V446 Cep 210478 109311 P EA 3.808       7.355 0.079 B1V
CW Cep 218066 113907 P EA/DM 2.729       7.736 0.251 B1:V:var
mu.01 Sco 151890 82514 P EB/SD 1.446       2.957 0.273 B1.5IV+B
V436 Per 11241 8704 P EA/D 25.936       5.485 0.237 B1.5V
HX Vel 74455 42712 P EB? 1.124       5.417 0.044 B1.5Vn
u Her 156633 84573 P EB 2.051       4.785 0.404 B1.5Vp
pi.05 Ori 31237 22797 P EB? 3.700       3.641 0.058 B2III SB
MS CMa 56554 35168 P EA 6.171       7.095 0.098 B2III/IV
psi Ori 35715 25473 P EB 2.526       4.514 0.044 B2IV
V954 Sco 149779 81508 P EB 1.269       7.625 0.273 B2IV
V461 Car 66546 39225 P EA 2.515       6.119 0.067 B2IV-V
V1384 Ori 40005 28142 P EA 6.572       7.203 0.233 B2V
V1388 Ori 42401 29321 P EB 2.187       7.494 0.343 B2V
LZ CMa 54912 34579 P EB 3.309       5.635 0.044 B2V
MX CMa 57192 35461 P EB 2.486       6.757 0.065 B2V
QZ Pup 64503 38455 P EB 1.112       4.430 0.058 B2V
TU Mon   38523 P EB 5.049       9.286 0.183 B2Vn
XY Pyx 71801 41515 P EB 0.923       5.702 0.069 B2V
CV Vel 77464 44245 P EA/DM 6.889       6.692 0.424 B2V+B2V
V1040 Sco 142184 77859b P EB/SD 0.508 0.508 1.017   5.398 0.037 B2V
V539 Ara 161783 87314 P EA/DM 3.169       5.699 0.372 B2V+B3V
V599 Aql 176853 93502 P EB 1.846       6.707 0.044 B2V
V1773 Cyg 193536 100142 P EB? 2.985       6.423 0.055 B2V
V1792 Cyg 198784 102953 P EB 3.303       7.308 0.100 B2V
V383 Cep 208106 107913 P EB 1.496       7.454 0.328 B2Vnp
V470 Cyg 228911 100193d P EB 1.873       8.550 0.055 B2+...
V427 Cep 239676 105960d P EB 1.911       9.223 0.117 B2
NO Vel 69144 40285 P EB 4.823       5.090 0.035 B2.5IV
IT Lib 138503 76161 P EB 2.267       9.111 0.522 B2/3IV:n:
AN Dor 31407 22663d P EA 2.033       7.621 0.136 B2/B3V
V4197 Sgr 177559 93785 P EW 0.715       8.253 0.648 B2/3V(n)
V393 Sco 161741 87191 P EB 7.713       7.613 0.674 B3III
HY Vel 74560 42726d P   3.102       4.773 0.055 B3IV
V360 Lac 216200 112778 P   10.082       5.943 0.063 B3IV:var
AR Cas 221253 115990 P   6.066       4.849 0.039 B3IV
lam Tau 25204 18724 P   3.953       3.395 0.128 B3V+A
EO Aur 34333 24744 P EB/SD 4.066       7.871 0.541 B3V+B3V
WX Lep 37622 26612 P EB 1.840       7.966 0.088 B3Vn
AE Pic 46792 31068 P EB 2.982       6.103 0.057 B3V
  47247 31593b U EA   0.993 1.986 2.095 6.315 0.093 B3V
V462 Car 66768 39310 P EB/IA 1.106       6.724 0.166 B3V(n)
V438 Pup 71302 41250c U EA?   1.183     5.918 0.139 B3V
QX Car 86118 48589 P EA/DM 4.478       6.626 0.395 B3V+B3V
V345 Vel 90000 50780 P EA 10.495       7.528 0.211 B3V
V3894 Sgr 161756 87163 P EB 2.619       6.352 0.130 B3Vn
V1441 Aql 177624 93732 P EB 2.374       6.937 0.102 B3V
sig Aql 185507 96665 P EB 1.950       5.195 0.125 B3V+B3V
MR Cyg   108508 P EB 1.677       8.881 0.524 B3V
GT Cep 217224 113385 P EA/SD 4.909       8.279 0.629 B3V
FZ CMa 52942 33953 P EA 1.273       8.170 0.284 B3n
AO Mon 53883 34299 P EA 1.885       9.676 0.547 B3+B5
V2126 Cyg 235271 101439 P EB 5.891       9.023 0.134 B3
RS Sgr 167647 89637 P EB 2.416       6.025 0.209 B3/B4IV/V
FF CMa 55173 34646 P EB/KE 1.213       7.468 0.444 B3/5V(p)
zet Phe 6882 5348 P EA/DM 1.670       3.953 0.304 B6V+B0V
          OBe   Total : 7        
V1036 Sco 159176 86011 P EB? 3.367       5.705 0.040 O5/6(e)
V1007 Sco 152248 82691 P EA 5.817       6.125 0.127 O7e
V729 Cyg   101341 P EB/D/G 6.597       9.139 0.278 O7e
SX Aur 33357 24201 P EB/KE 1.210       8.518 0.482 B1:V:ne:
AI Cru   59026 P EB 1.418       9.645 0.631 B2IVe
GU CMa 52721 33868 P EB 1.610       6.579 0.214 B2Vne
IU Aur 35652 25565 P EB/SD 1.811       8.439 0.546 B3Vnne
          OBSG   Total : 26        
V884 Sco 153919 83499 P EB 3.411       6.573 0.066 O5f
UW CMa 57060 35412 P EB/KE: 4.393       4.904 0.421 O7f
MY Ser 167971 89681 P EB 3.322       7.549 0.237 O8/9f
V918 Sco 149404 81305 P EA? 9.813       5.540 0.037 O9Ia
tau CMa 57061 35415 P EW/GS 1.282       4.336 0.058 O9Ib
V453 Sco 163181 87810 P EB/GS 12.006       6.684 0.413 O9.5Ia/ab
del Ori 36486 25930 P EA 5.732       2.148 0.097 O9.5II
QZ Car 93206 52526 P EB/GS 5.999       6.325 0.206 B0Ib:
V861 Sco 152667 82911 P EB/GS 7.848       6.260 0.260 B0.5Ia
GP Vel 77581 44368 P E 8.965       7.005 0.096 B0.5Ib
V1765 Cyg 187459 97485 P EA/GS 13.374       6.499 0.100 B0.5Ibvar
V373 Cas 224151 117957 P E 13.419       6.087 0.069 B0.5IIv SB
V421 Pup 68026 39968 P EB 5.417       9.093 0.145 B1II
QR Ser 168183 89753 P EB: 4.016       8.313 0.112 B1Ib/II
V448 Cyg 190967 99021 P EB 6.520       8.216 0.602 B1Ib-II
FY Vel 72754 41882 P EB:/GS 33.840       6.944 0.264 B2Iape
V390 Pup 62747 37751 P EA 3.928       5.556 0.059 B2II
V399 Pup 64014 38186 P EA 3.910       9.343 0.222 B2II
FM CMa 53756 34221 P EA 2.789       7.306 0.258 B2/B3II
V1069 Sco 152504 82819 P EA 5.347       8.620 0.243 B2/B3II
V1081 Sco 158186 85569 P EA 8.770 8.770 1.957   7.004 0.099 B2/B3II
RZ Sct 169753 90382 P EA/GS 15.190       7.675 0.314 B3Ib
V368 Cas 19644 14936 P EA 4.452       8.365 0.438 B3II-III
V438 Per 13970 10704 P EB/GS? 3.509       8.360 0.092 B5Ib
V505 Mon 48914 32397 P EB/GS 53.781 53.780 30.303   7.231 0.249 B5Ib
MP TrA 143028 78526b,c U EA   2.070   2.070c 7.789 0.099 B7Ib/II
      Total:       127        

Table A.1 is the complete version of Table 4. The columns are: the variable name, the HD number, the HIPPARCOS number, the HIPPARCOS variability flag, the variability type we assigned them in this study, the HIPPARCOS period (if any), the new periods found in this study (2 columns, for a possible second period), the periods found by Koen & Eyer (2002) (if any), the Hp magnitude, the mean amplitude calculated here and the spectral type according to the Vizier database.
a Koen et al. (2002); b This study; c Otero et al. (2003); d refers to the stars that were not included in the study or below $T_{\rm h}$.


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