Table 6
Clusters found for dwarf stars and their real open clusters using five components.
| Coverage | Age | ||||
| Cluster | OC | Stars | Cluster | OC | (Gyr) |
|
|
|||||
| N. 01 D | IC 4651 | 6 | 100% | 100% | 1.14 |
|
|
|||||
| N. 02 D | M 67 | 8 | 89% | 29% | 4.09 |
| NGC 3680 | 1 | 11% | 50% | 1.19 | |
|
|
|||||
| N. 03 D | Melotte111 | 4 | 57% | 80% | 0.71 |
| IC 4756 | 1 | 14% | 100% | 0.67 | |
| Melotte20 | 1 | 14% | 100% | 0.06 | |
| NGC 6475 | 1 | 14% | 100% | 0.25 | |
|
|
|||||
| N. 04 D | Melotte111 | 1 | 25% | 20% | 0.71 |
| Melotte22 | 1 | 25% | 100% | 0.11 | |
| NGC 2547 | 1 | 25% | 100% | 0.04 | |
| NGC 3680 | 1 | 25% | 50% | 1.19 | |
|
|
|||||
| N. 05 D | M 67 | 12 | 100% | 43% | 4.09 |
|
|
|||||
| N. 06 D | M 67 | 4 | 100% | 14% | 4.09 |
|
|
|||||
| N. 07 D | M 67 | 2 | 100% | 7% | 4.09 |
|
|
|||||
| N. 08 D | M 67 | 2 | 100% | 7% | 4.09 |
|
|
|||||
| N. 09 D | NGC 2447 | 3 | 100% | 100% | 0.56 |
|
|
|||||
| N. 10 D | NGC 2632 | 7 | 100% | 64% | 0.63 |
|
|
|||||
| N. 11 D | NGC 2632 | 4 | 100% | 36% | 0.63 |
Notes. The clustering algorithm assigns numbers to each identified group as indicated in the first column. The number of stars are presented next to the real open cluster to which they belong. The coverage indicates the percentage of stars found by comparing the total number of stars in the identified group to the number in the real open cluster.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.