Table 2:
Derived parameters of the open cluster sample
Name |
 |
Ref. |
 |
Ref. |
 |
![$\log\,(L_V/M_{\rm dyn}) [{L}_{V,\odot}/{M}_\odot]$](/articles/aa/full/2008/48/aa10251-08/img15.gif) |
NGC 1976 |
5.90 |
38 |
 |
(9, 20), 29 |
 |
 |
NGC 2168 |
8.26 |
9, 18 |
 |
3, 20, 39, 42, 43, 47 |
 |
 |
NGC 2516 |
8.2 |
41 |
0.15 |
3, 6, 9, 20, (42, 43) |
 |
 |
NGC 2632 |
8.88 |
31 |
0.10 |
2, 9, 20, 31, 36, (39) |
 |
 |
NGC 2682 |
9.61 |
31 |
 |
9, 10, 14, 20, 31, 36 |
 |
 |
|
|
|
|
37, 39, 42, 43, 46 |
|
|
NGC 3532 |
8.42 |
31 |
 |
3, 5, 9, 20, 31 |
 |
 |
NGC 5662 |
7.89 |
31 |
 |
9, 20, 30, 31 |
 |
 |
|
|
|
|
34, 42, 43 |
|
|
NGC 6705 |
8.4 |
9, 40 |
0.1 |
3, (8), 20, 27 |
 |
 |
|
|
|
|
(30, 39), 42, 43 |
|
|
Pleiades |
7.90 |
31 |
 |
9, 20, 31, 39 |
 |
 |
Coma Ber |
8.72 |
31 |
 |
9, 20, 28, 31 |
 |
 |
Hyades |
8.85 |
31, 36 |
 |
9, 31, 39 |
 |
 |
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