Basel 10
(FSR 0586; OCL 349.1; Dolidze 47b; MWSC 176)
0.80
UTI
0.75
CN
1.0
Cdens
0.75
CC3
0.74
Clit
1.0
Cdup
Stellar density (N50/rad)
23.7 [N/pc2]
- CN 0.75 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.74 Moderately studied
- Cdup 1.0 Unique
Overview
Basel 10 is a rich, very dense object of high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the age and mass parameters (see Parameters). It is moderately studied in the literature.
Note: This object shares a small 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 | 99999β | 34.879 | 58.291 | 0.448 | -0.442 | -0.844 | -32.835 |
| Li et al. | 2025 | 34.878 | 58.304 | 0.442 | -0.48 | -0.815 | β |
| Almeida et al. | 2025 | 34.861 | 58.298 | β | β | β | β |
| Hunt & Reffert | 2024 | 34.865 | 58.294 | 0.442 | -0.449 | -0.865 | β |
| Cavallo et al. | 2024 | 34.883 | 58.291 | 0.441 | β | β | β |
| Hunt & Reffert | 2023 | 34.865 | 58.294 | 0.442 | -0.449 | -0.865 | β |
| Jaehnig et al. | 2021 | 34.862 | 58.301 | 0.473 | -0.423 | -0.796 | β |
| Rain et al. | 2021 | 34.878 | 58.304 | 0.442 | -0.48 | -0.815 | β |
| Dias et al. | 2021 | 34.861 | 58.298 | 0.44 | -0.476 | -0.83 | β |
| Cantat-Gaudin et al. | 2020 | 34.878 | 58.304 | 0.442 | -0.48 | -0.815 | β |
| SΓ‘nchez et al. | 2020 | 34.867 | 58.3 | β | -0.512 | -0.949 | β |
| Zhong et al. | 2020 | 34.878 | 58.304 | β | -0.48 | -0.815 | -24.958 |
| Cantat-Gaudin & Anders | 2020 | 34.878 | 58.304 | 0.442 | -0.48 | -0.815 | β |
| Bica et al. | 2019 | 34.87 | 58.305 | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 34.878 | 58.304 | 0.442 | -0.48 | -0.815 | β |
| Loktin & Popova | 2017 | 34.86 | 58.3 | β | -0.23 | 1.105 | -32.1 |
| Sampedro et al. | 2017 | 34.867 | 58.3 | 1.63 | 0.35 | β | β |
| Gozha et al. | 2012 | 34.867 | 58.3 | β | β | β | β |
| Bukowiecki et al. | 2011 | 34.842 | 58.302 | β | β | β | β |
| Froebrich et al. | 2007 | 34.862 | 58.294 | β | β | β | β |
| Ahumada & Lapasset | 2007 | 34.7 | 58.317 | β | β | β | β |
| van den Bergh | 2006 | 34.7 | 58.317 | β | β | β | β |
| Dias et al. | 2002 | 34.867 | 58.3 | β | 1.47 | 0.35 | -32.1 |
| Lynga | 1987 | 34.69 | 58.307 | β | β | β | β |
π‘ 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 | 99999β | 2.08 | 2.42 | 1.44 | 42 | 0.124 | 402 | β | 0 |
| Li et al. | 2025 | 1.90 | 2.03 | β | 364 | 0.144 | β | β | β |
| Almeida et al. | 2025 | 2.05 | 2.10 | β | 292 | β | 96 | β | β |
| Hunt & Reffert | 2024 | β | β | β | β | β | 681(1) | β | β |
| Cavallo et al. | 2024 | 2.22 | 2.35 | β | 166 | 0.350 | β | β | β |
| Hunt & Reffert | 2023 | 2.06 | 2.16 | 1.44 | 122 | β | β | β | β |
| Jaehnig et al. | 2021 | 2.10(1) | β | β | β | β | β | β | β |
| Rain et al. | 2021 | 2.12 | 2.43 | β | 40 | β | β | β | 0 |
| Dias et al. | 2021 | 2.05 | 2.10 | β | 292 | 0.104 | β | β | β |
| Cantat-Gaudin et al. | 2020 | 2.32 | 1.66 | β | 71 | β | β | β | β |
| Kounkel et al. | 2020 | 2.10 | 2.52 | β | 43 | β | β | β | β |
| Zhong et al. | 2020 | 2.12(1) | 2.44 | β | 7608 | 0.000 | β | β | β |
| Cantat-Gaudin & Anders | 2020 | 2.12 | β | β | β | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 2.12 | β | β | β | β | β | β | β |
| Loktin & Popova | 2017 | 1.91 | 2.42 | β | 36 | β | β | β | β |
| Bukowiecki et al. | 2012 | β | β | β | β | β | 402 | β | β |
| Gozha et al. | 2012 | 1.94 | β | β | 41 | β | β | β | β |
| Bukowiecki et al. | 2011 | 1.93(1) | 2.18 | β | 28 | β | β | β | β |
| Ahumada & Lapasset | 2007 | β | 2.43 | β | 41 | β | β | β | 0 |
| van den Bergh | 2006 | 1.94 | 2.43 | β | 41 | β | β | β | β |
| Dias et al. | 2002 | 1.94 | 2.44 | β | 41 | β | β | β | β |
| Lynga | 1987 | 2.60 | 3.34 | β | 16 | β | β | β | β |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Almeida et al. (2025)
Mass determination: worst fit. Isochrone match: intermediate fit.
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).
Bica et al. (2019)
Analysis of Dolidze objects by M. Kronberger reported in DAML02.