Berkeley 51
(FSR 0197; MWSC 3280; OCL 146)
0.82
UTI
0.79
CN
1.0
Cdens
0.75
CC3
0.78
Clit
1.0
Cdup
Stellar density (N50/rad)
40.9 [N/pc2]
- CN 0.79 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.78 Well-studied
- Cdup 1.0 Unique
Overview
Berkeley 51 is a rich, very dense object of high C3 quality. Its parallax locates it at a large distance, near the mid-plane, affected by very high extinction. It is catalogued as a massive, near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the mass parameter (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 | 302.977 | 34.403 | 0.156 | -3.059 | -4.868 | -23.534 |
| Hunt & Reffert | 2024 | 302.972 | 34.404 | 0.17 | -3.063 | -4.864 | -27.524 |
| Cavallo et al. | 2024 | 302.995 | 34.39 | 0.155 | â | â | â |
| Hunt & Reffert | 2023 | 302.972 | 34.404 | 0.17 | -3.063 | -4.864 | -27.524 |
| Just et al. | 2023 | 302.969 | 34.407 | â | â | â | â |
| Cantat-Gaudin et al. | 2020 | 302.972 | 34.402 | 0.167 | -3.066 | -4.918 | â |
| Cantat-Gaudin & Anders | 2020 | 302.972 | 34.402 | 0.167 | -3.066 | -4.918 | â |
| Soubiran et al. | 2018 | 302.972 | 34.402 | â | â | â | -23.5 |
| Bica et al. | 2019 | 302.988 | 34.398 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 302.972 | 34.402 | 0.167 | -3.066 | -4.918 | â |
| Kharchenko et al. | 2016 | 302.969 | 34.407 | â | â | â | â |
| Kharchenko et al. | 2013 | 302.974 | 34.41 | â | -1.15 | -1.37 | â |
| Bukowiecki et al. | 2011 | 302.967 | 34.404 | â | â | â | â |
| Froebrich et al. | 2007 | 302.971 | 34.413 | â | â | â | â |
| Dias et al. | 2002 | 302.975 | 34.402 | â | -1.15 | -1.37 | â |
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 | 5.1 | 5.475 | 2.81 | 180 | -0.250 | 3146 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 6904(1) | â | â |
| Cavallo et al. | 2024 | 3.89 | 5.31 | â | 102 | -0.250 | â | â | â |
| Hunt & Reffert | 2023 | 5.47 | 5.64 | 2.81 | 50 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 180 | â | 1274 | â | â |
| Cantat-Gaudin & Anders | 2020 | 5.10 | â | â | â | â | â | â | â |
| Soubiran et al. | 2018 | 5.10 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 5.10 | â | â | â | â | â | â | â |
| Kharchenko et al. | 2016 | 3.29 | 5.81 | â | 180 | â | â | â | â |
| Kharchenko et al. | 2013 | 3.29 | 5.81 | â | 180 | â | â | â | â |
| Bukowiecki et al. | 2012 | â | â | â | â | â | 3146 | â | â |
| Bukowiecki et al. | 2011 | 5.94(1) | 4.59 | â | 126 | â | â | â | â |
| Dias et al. | 2002 | 1.30 | 4.96 | â | 1122 | â | 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.