Berkeley 75
(MWSC 993; OCL 614; ES0490SC50)
0.88
UTI
0.77
CN
1.0
Cdens
1.0
CC3
0.81
Clit
1.0
Cdup
Stellar density (N50/rad)
9.4 [N/pc2]
- CN 0.77 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.81 Well-studied
- Cdup 1.0 Unique
Overview
Berkeley 75 is a rich, very dense object of very high C3 quality. Its parallax locates it at a large distance, well below the mid-plane, affected by low extinction. It is catalogued as a massive, near-solar metallicity, old cluster, but with a large variance across recent sources for the age, metallicity, and mass parameters (see Parameters). It is well-studied in the literature.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 102.251 | -23.996 | 0.104 | -0.232 | 1.147 | 125.075 |
| Hunt & Reffert | 2024 | 102.249 | -23.996 | 0.108 | -0.241 | 1.179 | 125.07 |
| Cavallo et al. | 2024 | 102.268 | -24.015 | 0.104 | â | â | â |
| Hunt & Reffert | 2023 | 102.249 | -23.996 | 0.108 | -0.241 | 1.179 | 125.07 |
| Just et al. | 2023 | 102.258 | -23.983 | â | â | â | â |
| Perren et al. | 2022 | 102.252 | -23.999 | â | â | â | â |
| Cantat-Gaudin et al. | 2020 | 102.252 | -23.999 | 0.088 | -0.264 | 1.088 | â |
| Cantat-Gaudin & Anders | 2020 | 102.252 | -23.999 | 0.088 | -0.264 | 1.088 | â |
| Soubiran et al. | 2018 | 102.252 | -23.999 | â | â | â | 126.82 |
| Bica et al. | 2019 | 102.259 | -23.987 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 102.252 | -23.999 | 0.088 | -0.264 | 1.088 | â |
| Loktin & Popova | 2017 | 102.255 | -23.996 | â | 0.418 | 1.254 | 94.6 |
| Kharchenko et al. | 2016 | 102.258 | -23.983 | â | â | â | â |
| Kharchenko et al. | 2013 | 102.264 | -23.985 | â | 0.51 | 5.35 | 94.6 |
| Gozha et al. | 2012 | 102.254 | -23.997 | â | â | â | â |
| Dias et al. | 2002 | 102.254 | -23.997 | â | -4.56 | -9.82 | 94.6 |
đĄ Note: The UCC values are estimated from its identified members.
| Reference | Year | Dist [kpc] | Av [mag] | DAv [mag] | Age [Myr] | [Fe/H] [dex] | Mass [Msun] | Bfrac | BSS |
|---|---|---|---|---|---|---|---|---|---|
| UCC | 99999â | 8.17 | 0.245 | 1.08 | 1995 | -0.220 | 2600 | 0.77 | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 583(1) | â | â |
| Cavallo et al. | 2024 | 4.37 | 0.80 | â | 11482 | -1.000 | â | â | â |
| Hunt & Reffert | 2023 | 7.44 | 0.20 | 1.08 | 1858 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 1995 | â | 2600 | â | â |
| Perren et al. | 2022 | 8.02 | 0.34 | â | 5495 | -0.390 | 6800 | 0.77 | â |
| Cantat-Gaudin et al. | 2020 | 8.32 | 0.29 | â | 1698 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 8.51 | â | â | â | â | â | â | â |
| Soubiran et al. | 2018 | 8.51 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 8.51 | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 3.52 | 0.95 | â | 1738 | â | â | â | â |
| Kharchenko et al. | 2016 | 6.27 | 0.12 | â | 1995 | â | â | â | â |
| Kharchenko et al. | 2013 | 6.27 | 0.12 | â | 1995 | -0.220 | â | â | â |
| Gozha et al. | 2012 | 9.10 | â | â | 3981 | -0.220 | â | â | â |
| Dias et al. | 2002 | 9.10 | 0.12 | â | 3981 | -0.220 | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Cavallo et al. (2024)
Silver sample.