Free Access
Table 5
List of previously studied open clusters.
| Cluster | Stars | Type | Ref. | |
|
|
||||
| NGC 188 | 13 | MS | Norris & Smith (1985) | |
| NGC 188 | 7 | RC/RGB | Martell & Smith (2009) | |
| NGC 2158 | 6 | RC/RGB | Martell & Smith (2009) | |
| NGC 2158 | 10 | RC | Smith & Norris (1984) | |
| NGC 6791a | 31 | RC/RGB | Hufnagel et al. (1995) | |
| NGC 6791 | 97 | MS/RGB/RC | Paper I | |
| NGC 7789 | 10 | RC/RGB | Martell & Smith (2009) | |
Notes.
(a)
Although Hufnagel et al. (1995) found evidence of variations in the CN band strengths among the stars in their sample, they did not associate them with the existence of star-to-star abundance variations.
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.