Table 3:
Field O stars possibly associated with young clusters. See Tables 1 and 2 for the meaning of the abbreviations used in Cols. 2 and 3. The
projected distance is with respect to the distance of the field O star.
Name |
VM |
SM |
Proj. dist. |
Cluster |
Age |
Ref. |
|
|
|
(pc) |
|
(Myr) |
|
HD 117856 |
VB |
SB2: |
57 |
St 16 |
4 |
1 |
HD 125206 |
single |
SB2: |
45 |
NGC 5606 |
7 |
2 |
HD 154368 |
VB |
SBE |
42 |
Bo 13 |
6.3 |
3 |
HD 154643 |
single |
SB1: |
44 |
Bo 13 |
6.3 |
3 |
HD 158186 |
single |
SBE |
30 |
NGC 6383 |
1.7 |
4 |
HD 161853 |
single |
SB1: |
55 |
Col 347 |
6.3 |
3 |
HD 169515 |
single |
SB2OE |
65 |
NGC 6604 |
4 |
3 |
1:
Turner 1985; 2:
Vazquez et al. (1994); 3:
Battinelli et al. (1994); 4:
Fitzgerald et al. (1978).
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