Berkeley 20
(MWSC 572; OCL 497)
0.96
UTI
0.8
CN
1.0
Cdens
1.0
CC3
1.0
Clit
1.0
Cdup
Radius (P>50% members)
1.3 [arcmin]
- CN 0.8 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
Berkeley 20 is a rich, very dense object of very high C3 quality. Its parallax locates it at a very large distance, well below the mid-plane, affected by low extinction. It is catalogued as a massive, metal-poor, very old cluster, but with a large variance across recent sources for the distance, age, metallicity, and mass parameters (see Parameters). It is very well-studied in the literature.
Note: This object contains blue stragglers according to at least one source.
Very distant
Low extinction
Massive
Metal-poor
Very old
Contains BSS
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 83.153 | 0.186 | 0.1 | 0.869 | -0.231 | 79.133 |
| Zhang et al. | 2024 | 83.154 | 0.188 | â | â | â | â |
| Hunt & Reffert | 2024 | 83.154 | 0.188 | 0.094 | 0.827 | -0.246 | 78.888 |
| Cavallo et al. | 2024 | 83.142 | 0.177 | 0.116 | â | â | â |
| Hunt & Reffert | 2023 | 83.154 | 0.188 | 0.094 | 0.827 | -0.246 | 78.888 |
| Just et al. | 2023 | 83.147 | 0.184 | â | â | â | â |
| Jaehnig et al. | 2021 | 83.155 | 0.189 | 0.045 | 0.82 | -0.259 | â |
| Rain et al. | 2021 | 83.152 | 0.185 | 0.04 | 0.808 | -0.244 | â |
| Cantat-Gaudin et al. | 2020 | 83.152 | 0.185 | 0.04 | 0.808 | -0.244 | â |
| Donor et al. | 2020 | 83.154 | 0.183 | â | 1.04 | -0.16 | 78.8 |
| Cantat-Gaudin & Anders | 2020 | 83.152 | 0.185 | 0.04 | 0.808 | -0.244 | â |
| Bica et al. | 2019 | 83.16 | 0.184 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 83.152 | 0.185 | 0.04 | 0.808 | -0.244 | â |
| Loktin & Popova | 2017 | 83.16 | -0.188 | â | 1.51 | -4.11 | 75.7 |
| Kharchenko et al. | 2016 | 83.147 | 0.184 | â | â | â | â |
| Kharchenko et al. | 2013 | 83.154 | 0.183 | â | -1.62 | -4.26 | 75.7 |
| Gozha et al. | 2012 | 83.154 | 0.188 | â | â | â | â |
| Kharchenko et al. | 2007 | 83.16 | 0.19 | â | 0.02 | â | â |
| van den Bergh | 2006 | 83.25 | 0.217 | â | â | â | â |
| Chen et al. | 2003 | 83.248 | 0.21 | â | â | â | â |
| Dias et al. | 2002 | 83.154 | 0.188 | â | 1.51 | -4.11 | 70.0 |
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] | Bfr | BSS |
|---|---|---|---|---|---|---|---|---|---|
| Zhang et al. | 2024 | â | â | â | â | -0.355* | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 834* | â | â |
| Cavallo et al. | 2024 | 4.02 | 1.35 | â | 6166 | -0.720 | â | â | â |
| Hunt & Reffert | 2023 | 7.99 | 0.46 | 1.69 | 1841 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 6026 | â | 2972 | â | â |
| Jaehnig et al. | 2021 | 14.23* | â | â | â | â | â | â | â |
| Rain et al. | 2021 | 14.40 | 0.37 | â | 6026 | â | â | â | 6 |
| Cantat-Gaudin et al. | 2020 | 8.71 | 0.37 | â | 4786 | â | â | â | â |
| Donor et al. | 2020 | â | â | â | â | -0.400 | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 14.40 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 14.40 | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 8.80 | 4.65 | â | 5358 | â | â | â | â |
| Kharchenko et al. | 2016 | 8.40 | 0.38 | â | 6026 | â | â | â | â |
| Kharchenko et al. | 2013 | 8.40 | 0.38 | â | 6026 | -0.610 | â | â | â |
| Gozha et al. | 2012 | 8.40 | â | â | 6026 | -0.610 | â | â | â |
| van den Bergh | 2006 | 8.40 | 0.37 | â | 6026 | â | â | â | â |
| Chen et al. | 2003 | 8.40 | 0.37 | â | 6020 | -0.750* | â | â | â |
| Dias et al. | 2002 | 8.40 | 0.37 | â | 6026 | -0.300 | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Silver sample.