Table 1
Comparison between BSS astrophysical parameters obtained in this study against those found in the literature.
| Name | NBSS | ⟨ Teff⟩ | ⟨log(g)⟩ | ⟨Mass⟩ | Reference | |
|---|---|---|---|---|---|---|
| (K) | (M⊙) | |||||
| Open Clusters | ||||||
| NGC 188 | 19 | 6396 ± 233 | – | – | Gosnell et al. (2015) | |
| 21 | 6366 ± 496 | – | – | This Work – IRFM | ||
| 21 | 6473 ± 416 | 4.05 ± 0.17 | 1.45 ± 0.17 | This Work – isochrone | ||
| NGC 2682 | 21 | 6510 ± 429 | – | – | Jadhav et al. (2019) | |
| 3 | 8333 ± 721 | – | – | Sindhu et al. (2019) | ||
| 6 | 7291 ± 485 | 3.67 ± 0.52 | – | Pandey et al. (2021) | ||
| 9 | 7308 ± 1220 | – | – | This Work – IRFM | ||
| 9 | 7287 ± 1015 | 4.08 ± 0.20 | 1.70 ± 0.39 | This Work – isochrone | ||
| NGC 7789 | 15 | 8433 ± 961 | 4.23 ± 0.46 | – | Vaidya et al. (2022) | |
| 16 | 8690 ± 1142 | – | – | This Work – IRFM | ||
| 16 | 8469 ± 1008 | 3.93 ± 0.22 | 2.03 ± 0.31 | This Work – isochrone | ||
| Multiple OCs | 1368 | – | – | 2.49 ± 1.13 | Jadhav & Subramaniam (2021) | |
| 434 | 7598 ± 1476 | – | – | This Work – IRFM | ||
| 434 | 7549 ± 1331 | 3.98 ± 0.21 | 1.75 ± 0.45 | This Work – isochrone | ||
| Globular Clusters | ||||||
| NGC 362 | 26 | 7810 ± 863 | 4.29 ± 0.53 | – | Dattatrey et al. (2023) | |
| 137 | 6718 ± 465 | – | – | This Work – IRFM | ||
| NGC 5272 | 137 | 6816 ± 405 | 4.09 ± 0.20 | 0.94 ± 0.08 | This Work – isochrone | |
| 7 | 7093 ± 917 | 3.61 ± 0.58 | – | De Marco et al. (2005) | ||
| 210 | 6910 ± 621 | – | – | This Work – IRFM | ||
| 210 | 6978 ± 520 | 4.11 ± 0.22 | 0.98 ± 0.10 | This Work – isochrone | ||
| NGC 6541 | 9 | – | – | 1.06 ± 0.09 | Fiorentino et al. (2014) | |
| 52 | 7240 ± 760 | 4.09 ± 0.26 | 1.00 ± 0.10 | This Work – isochrone | ||
| Multiple GCs | 64 | 6969 ± 967 | – | 1.11 ± 0.09 | Stępień & Kiraga (2015) | |
| 598 | – | – | 1.22 ± 0.12 | Baldwin et al. (2016) | ||
| 1507 | – | – | 1.07 ± 0.13 | Simunovic (2017) | ||
| 3965 | 6772 ± 630 | – | – | This Work – IRFM | ||
| 3965 | 6829 ± 529 | 4.14 ± 0.22 | 1.02 ± 0.01 | This Work – isochrone | ||
Notes. Columns are as follows: (1) Cluster name. (2) Number of available BSSs in the literature with available astrophysical parameters. (3) Mean of the effective BSS temperature provided. (4) Mean of the decadal logarithm of the BSS surface gravity. (5) Mean of the BSS stellar mass. (6) Reference. For data provided by Jadhav & Subramaniam (2021, or JS21), we considered stars labeled BSS and pBSS (probable BSS).
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