Table 3.
N-rich stars and potential GC origin from Method I.
| Gaia EDR3 ID | GC | Confidence (p) | m.e. (1) |
|---|---|---|---|
| 4565255983145857920 | NGC 5139 | 0.41 | GE/Seq |
| 4553384792324044928 | NGC 5897 | 0.44 | GE |
| 4553384792324044928 | NGC 6355 | 0.42 | ... |
| 4553384792324044928 | NGC 6652 | 0.35 | ... |
| 4553384792324044928 | NGC 6809 | 0.58 | ... |
| 4526616017814192768 | NGC 6544 | 0.38 | ... |
| 4457311841406602752 | NGC 5946 | 0.36 | ... |
| 4457311841406602752 | NGC 6284 | 0.40 | GE |
| 4452741961844020992 | NGC 6712 | 0.56 | ... |
| 3903971791408436352 | NGC 2419 | 0.37 | Sag |
| 3903971791408436352 | NGC 5272 | 0.48 | H99 |
| 3903971791408436352 | Pal 5 | 0.43 | H99? |
| 3903971791408436352 | NGC 6235 | 0.34 | GE |
| 3903971791408436352 | NGC 6715 | 0.82 | Sag |
| 3903971791408436352 | Ter 8 | 0.50 | Sag |
| 3628877246314114176 | Pal 11 | 0.44 | ... |
| 3628603811516372864 | NGC 6235 | 0.61 | GE |
| 2485902851604869504 | NGC 4147 | 0.57 | GE |
| 2105942793032574592 | NGC 6352 | 0.36 | ... |
| 2095506851436919296 | NGC 6121 | 0.52 | ... |
| 1542187382923726848 | NGC 5139 | 0.40 | GE/Seq |
| 1314804426927128960 | NGC 6121 | 0.46 | ... |
| 1189399628220805760 | NGC 288 | 0.48 | GE |
| 1189399628220805760 | NGC 6325 | 0.38 | ... |
| 1189399628220805760 | NGC 6779 | 0.87 | G-E |
| 915304504835769216 | NGC 5904 | 0.45 | GE/H99 |
| 915304504835769216 | NGC 6584 | 0.70 | ... |
| 912107709138952192 | NGC 2419 | 0.39 | Sag |
| 912107709138952192 | Ter 8 | 0.74 | Sag |
Notes. The columns list the Gaia EDR3 star ID and cluster name, the confidence measured from full action distribution combining the metallicity, and the merger events. Entries in bold are the five most probable associations.
Merger events (m.e.) that might be associated with the host GCs (Massari et al. 2019). GE stands for Gaia-Enceladus (Helmi et al. 2018); Sag stands for Sagittarius dwarf (Ibata et al. 1994); H99 stands for Helmi Streams (Helmi et al. 1999); Seq stands for Sequoia galaxy (Myeong et al. 2019).
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