Table A.1
Current evolutionary masses for the sample stars, derived from the classical (M1) and the spectroscopic (M2) HRDs.
| Object | ST | Bonn tracks | Geneva tracks | Notes | ||
|---|---|---|---|---|---|---|
| M1 | M2 | M1 | M2 | |||
| HD 64568a | O3 V | 68.2 |
82 ± 20.5 | 68.0 |
74.8 |
|
| HD 46223 | O4 V | 47.0 |
51.8 |
47.3 |
46.5 |
|
| HD 93843a | O5 III | 58.8 |
52.8 |
43.6 |
38.9 |
SB1? |
| CD−47 4551 | O5 If | 88 (ul) | 53.4 |
66.2 |
34.2 |
SB2 |
| HD 93204a | O5.5 V | 48.0 |
41.4 |
39.3 |
38.5 |
|
| CPD−59 2600a | O6 V | 36.7 |
35.4 |
36.1 |
35.0 |
SB1 |
| HD 91572a | O6.5 V | 34.0 |
34.6 |
32.8 |
32.8 |
SB1 |
| HD 63005a | O6.5 IV | 38.9 |
42.2 |
34.2 |
34.2 |
|
| HD 91824a | O7 V | 35.1 |
36.1 |
33.9 |
34.2 |
SB1 |
| CPD−58 2620a | O7 V | 28.1 |
32.9 |
27.7 |
31.8 |
|
| HD 93222 | O7 V | 33.8 |
33.2 |
32.2 |
31.5 |
|
| HD 94963a | O7 II | 35.5 |
49.4 |
30.8 |
32.4 |
SB2? |
| HD 94963b | 41.0 |
49.5 |
32.2 |
32.4 |
||
| HD 94370a | O7 | 32.4 |
33.9 |
29.9 |
29.8 |
SB2? |
| HD 94370b | 36.2 |
34.1 |
31.0 |
29.9 |
||
| HD 151804 | O8 Iaf | 56.9 |
52.0 |
38.1 |
31.0 |
SB2 |
| HD 92504 | O8.5 V | 24.0 |
26.0 |
23.9 |
25.2 |
|
| HD 75211 | O8.5 II | 37.3 |
38.0 |
31.8 |
29.1 |
SB1 |
| HD 152249 | OC9 Iab | 36.8 |
51.5 |
29.5 |
30.9 |
|
| HD 46202 | O9.2 V | 22.0 |
21.9 |
21.8 |
21.6 |
|
| CD−44 4865 | O9.7 III | 26.9 |
28.3 |
24.5 |
24.6 |
|
| HD 152003 | O9.7 Iab | 39.6 |
49.9 |
30.8 |
30.8 |
|
| HD 75222 | O9.7 Iab | 35.4 |
47.4 |
28.6 |
29.5 |
SB? |
| HD 75222a | 39.8 |
47.4 |
30.8 |
29.5 |
||
| HD 78344 | O9.7 Iab | 39.8 |
46.7 |
30.8 |
29.4 |
|
| HD 169582 | O6 Iaf | 82 (ul) | 58.6 |
48.7 |
40.2 |
|
| CD−43 4690 | O6.5 III | 39.9 |
45.3 |
32.1 |
32.4 |
|
| HD 97848 | O8 V | 26.5 |
28.9 |
25.8 |
28.0 |
|
| HD 69464 | O7 Ib | 48.4 |
49.7 |
36.8 |
32.4 |
|
| HD 302505 | O8.5 III | 33.2 |
33.6 |
28.7 |
27.8 |
|
| HD 148546 | O9 Iab | 41.4 |
47.5 |
31.1 |
29.8 |
|
| HD 76968a | O9.2 Ib | 36.2 |
43.1 |
29.2 |
30.2 |
SB1 |
| HD 69106 | O9.7 II | 22.0 |
22.4 |
21.8 |
21.8 |
|
Notes. Cluster and association members are listed in the upper part, field stars in the lower part. Errors shown in italics are not derived but adopted values. “ul” means upper limit. For more information, see Sect. 5.2.
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