Table 6
Summary of known binaries and candidate radial-velocity variables in the AAOmega sample.
| Star | Spectral classification | AAΩ status | OGLE LMC-ECL | POGLE [d] | TypeOGLE |
|
|
|||||
| 010 | O9.5: + early B | SB2 | ... | ... | ... |
| 021 | B0.5: + early B | SB2 | 16629 | 2.923299 | EC |
| 024 | B1.5 Ib Nwk | ... | 16646 | 26.225620 | ED |
| 027 | B0.5: + early B | SB2 | 16675 | 3.748640 | ED |
| 038 | B1-1.5 V-III | ... | 16881 | 3.167171 | ED/VAR |
| 053 | B0.5 Ib Nwk | SB1 | ... | ... | ... |
| 058 | B1-1.5 V-III | ... | 17198 | 3.290830 | ED |
| 065 | O9.2-9.5 V | ... | 17334 | 1.362346 | ESD |
| 084 | B1.5 Ib Nwk | RV var? | 17823 | 4.585031 | EC |
| 085 | B0 V | RV var? | ... | ... | ... |
| 114 | B0.2 III: + early B | SB2 | ... | ... | ... |
| 122 | O9.5 III + B0: | SB2 | 18794 | 5.946846 | ED |
| 130 | B0.2: + early B | SB2 | ... | ... | ... |
| 135 | B1.5 III-II | RV var? | ... | ... | ... |
| 160 | B1.5 V-III | RV var? | ... | ... | ... |
| 173 | B0.5 Ib Nwk? | SB2? | 19892 | 4.682925 | ED |
| 178 | O6 V((f)) | ... | 19996 | 1.079433 | ED |
| 192 | O8.5 IIn | RV var? | ... | ... | ... |
| 267 | O9.5: II + early B | SB2 | 20901 | 1.554470 | ED |
| 330 | O9: V-III + O9.5: V-III | SB2 | 21568 | 3.225450 | ED |
| 337 | O9: V-III + O9.7: V-III | SB2 | ... | ... | ... |
| 352 | Mid-O V | ... | 21844 | 100.374558 | ED |
| 371 | O9.5 II | ... | 22166 | 1.759227 | ED |
| 374 | Early B + early B | SB2 | 22270 | 5.414011 | ED |
| 381 | O9 III | ... | 22429 | 100.032930 | ED/VAR |
| 414 | O8.5 Iabf (+ OB?) | SB2 | ... | ... | ... |
| 419 | B1-1.5 I | RV var? | ... | ... | ... |
Notes. Details of eclipsing binaries known from the OGLE survey are from Graczyk et al. (2011); classifications of light-curve variability in the final column are: EC = contact eclipsing binary; ED = detached eclipsing binary; ESD = semi-detached eclipsing binary; ED/VAR = detached with additional variability superimposed. Classifications of the spectra for AAΩ 30 Dor 084 and 374 were given by Muraveva et al. (2014), identified in their Table A3 as lm0020n19615 and lm0031122987, respectively; the more detailed classifications given here now supercede those.
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