Basel 4
(FSR 0825; Czernik22; MWSC 672; OCL 455)
0.82
UTI
0.76
CN
0.69
Cdens
1.0
CC3
0.84
Clit
1.0
Cdup
Nm (P>50%)
123
Core radius and density
2.1 [pc], 3.4 [pc-2]
- CN 0.76 Rich
- Cdens 0.69 Moderately dense
- CC3 1.0 Very high quality
- Clit 0.84 Well-studied
- Cdup 1.0 Unique
Overview
Basel 4 is a rich, moderately dense object of very high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is well-studied in the literature.
Note: This object shares a moderate percentage of members with a later reported entry. See table with shared members information.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 87.242 | 30.194 | 0.293 | 0.837 | -1.79 | 6.157 |
| Li et al. | 2025 | 87.242 | 30.19 | 0.286 | 0.835 | -1.801 | â |
| Almeida et al. | 2025 | 87.235 | 30.194 | â | â | â | â |
| Zhang et al. | 2024 | 87.243 | 30.192 | â | â | â | â |
| Hunt & Reffert | 2024 | 87.243 | 30.192 | 0.3 | 0.821 | -1.792 | 4.541 |
| Cavallo et al. | 2024 | 87.242 | 30.196 | 0.299 | â | â | â |
| Hunt & Reffert | 2023 | 87.243 | 30.192 | 0.3 | 0.821 | -1.792 | 4.541 |
| Just et al. | 2023 | 87.242 | 30.206 | â | â | â | â |
| Netopil et al. | 2022 | 87.242 | 30.189 | 0.278 | 0.846 | -1.804 | 6.52 |
| Dias et al. | 2021 | 87.235 | 30.194 | 0.279 | 0.837 | -1.809 | 6.533 |
| Cantat-Gaudin et al. | 2020 | 87.242 | 30.19 | 0.286 | 0.835 | -1.801 | â |
| Zhong et al. | 2020 | 87.242 | 30.19 | â | 0.835 | -1.801 | 4.466 |
| Cantat-Gaudin & Anders | 2020 | 87.242 | 30.19 | 0.286 | 0.835 | -1.801 | â |
| Bossini et al. | 2019 | 87.242 | 30.19 | â | â | â | â |
| Soubiran et al. | 2018 | 87.242 | 30.19 | â | â | â | 6.52 |
| Bica et al. | 2019 | 87.221 | 30.196 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 87.242 | 30.19 | 0.286 | 0.835 | -1.801 | â |
| Dias et al. | 2018 | â | â | â | 2.48 | -1.34 | â |
| Kharchenko et al. | 2016 | 87.242 | 30.206 | â | â | â | â |
| Dias et al. | 2014 | 87.125 | 30.217 | â | -0.59 | -2.65 | â |
| Kharchenko et al. | 2013 | 87.25 | 30.205 | â | -1.38 | -6.37 | â |
| Kharchenko et al. | 2012 | 87.25 | 30.205 | â | -1.38 | -6.37 | â |
| Bukowiecki et al. | 2011 | 87.237 | 30.182 | â | â | â | â |
| Froebrich et al. | 2007 | 87.237 | 30.173 | â | â | â | â |
| van den Bergh | 2006 | 87.125 | 30.217 | â | â | â | â |
| Dias et al. | 2002 | 87.125 | 30.217 | â | -0.59 | -2.65 | â |
| Lynga | 1987 | 87.126 | 30.217 | â | â | â | 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 | 3.04 | 1.58 | 0.89 | 288 | -0.175 | 670 | â | â |
| Li et al. | 2025 | 2.85 | 1.64 | â | 288 | -0.058 | â | â | â |
| Almeida et al. | 2025 | 2.83 | 1.78 | â | 198 | â | 320 | â | â |
| Zhang et al. | 2024 | â | â | â | â | -0.153(1) | â | â | â |
| Hunt & Reffert | 2024 | 2.95 | 1.33 | 0.89 | 339 | â | 975(1) | â | â |
| Cavallo et al. | 2024 | 2.42 | 1.58 | â | 457 | -0.290 | â | â | â |
| Hunt & Reffert | 2023 | 2.95 | 1.33 | 0.89 | 339 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 462 | â | 366 | â | â |
| Netopil et al. | 2022 | 3.60(1) | 1.74 | â | 158 | -0.180(1) | â | â | â |
| Dias et al. | 2021 | 2.83 | 1.78 | â | 198 | -0.175 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 3.33 | 1.48 | â | 112 | â | â | â | â |
| Kounkel et al. | 2020 | 3.04 | 1.67 | â | 295 | â | â | â | â |
| Zhong et al. | 2020 | 3.17(1) | 1.58 | â | 8665 | -0.275 | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 3.17 | â | â | â | â | â | â | â |
| Bossini et al. | 2019 | 3.40 | 1.52 | â | 136 | 0.000 | â | â | â |
| Soubiran et al. | 2018 | 3.17 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 3.17 | â | â | â | â | â | â | â |
| Kharchenko et al. | 2016 | 2.80 | 1.58 | â | 462 | â | â | â | â |
| Kharchenko et al. | 2013 | 2.80 | 1.58 | â | 462 | â | â | â | â |
| Bukowiecki et al. | 2012 | â | â | â | â | â | 2029 | â | â |
| Kharchenko et al. | 2012 | 2.80 | 1.58 | â | 462 | â | â | â | â |
| Bukowiecki et al. | 2011 | 3.07(1) | 1.42 | â | 178 | â | â | â | â |
| van den Bergh | 2006 | 5.67 | 1.67 | â | 10 | â | â | â | â |
| Dias et al. | 2002 | 3.00 | 1.42 | â | 200 | â | â | â | â |
| Lynga | 1987 | 5.90 | 2.02 | â | 13 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Almeida et al. (2025)
Mass determination: good fit. Isochrone match: good fit. Silver sample.
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as open cluster. CMD class: 1.00 (50th percentile).
Hunt & Reffert (2023)
Classified as open cluster. CMD class: 1.00 (50th percentile).
Hu et al. (2021)
Ellipticities (core, all): e_core=0.208, e_all=0.1216.