Stock 12
(MWSC 3743; OCL 258; FoF 2399; OCSN 267)
0.96
UTI
0.8
CN
1.0
Cdens
1.0
CC3
1.0
Clit
1.0
Cdup
Radius (P>50% members)
28.4 [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
Stock 12 is a rich, very dense object of very high C3 quality. Its parallax locates it at a very close distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the age and metallicity parameters (see Parameters). It is very well-studied in the literature.
Very close
Low extinction
Near-solar metallicity
Intermediate age
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 353.892 | 52.645 | 2.281 | 8.556 | -1.89 | -4.172 |
| Li et al. | 2025 | 353.923 | 52.685 | 2.261 | 8.527 | -1.846 | â |
| Almeida et al. | 2025 | 353.978 | 52.698 | â | â | â | â |
| Alfonso et al. | 2024 | -5.941 | 52.69 | 2.27 | 8.513 | -2.006 | â |
| Zhang et al. | 2024 | 353.87 | 52.623 | â | â | â | â |
| Hunt & Reffert | 2024 | 353.87 | 52.623 | 2.287 | 8.571 | -1.917 | -3.151 |
| Cavallo et al. | 2024 | 353.946 | 52.634 | 2.289 | â | â | â |
| Hunt & Reffert | 2023 | 353.87 | 52.623 | 2.287 | 8.571 | -1.917 | -3.151 |
| Cordoni et al. | 2023 | 353.978 | 52.698 | 2.257 | 8.547 | -1.857 | â |
| Qin et al. | 2023 | 353.99 | 52.66 | 2.29 | 8.53 | -1.93 | -4.63 |
| Just et al. | 2023 | 353.887 | 52.682 | â | â | â | â |
| He et al. | 2022 | 354.008 | 52.713 | 2.28 | 8.535 | -1.883 | â |
| Tarricq et al. | 2022 | 353.803 | 52.649 | 2.269 | 8.522 | -1.869 | â |
| Dias et al. | 2021 | 353.978 | 52.698 | 2.257 | 8.547 | -1.857 | -3.469 |
| Cantat-Gaudin et al. | 2020 | 353.923 | 52.685 | 2.261 | 8.527 | -1.846 | â |
| Cantat-Gaudin & Anders | 2020 | 353.923 | 52.685 | 2.261 | 8.527 | -1.846 | â |
| Liu & Pang | 2019 | 354.006 | 52.72 | 2.256 | 8.519 | -1.853 | â |
| Bossini et al. | 2019 | 353.923 | 52.685 | â | â | â | â |
| Soubiran et al. | 2018 | 353.923 | 52.685 | â | â | â | -4.2 |
| Bica et al. | 2019 | 354.108 | 52.522 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 353.923 | 52.685 | 2.261 | 8.527 | -1.846 | â |
| Loktin & Popova | 2017 | 354.09 | 52.543 | â | 7.55 | -2.07 | -18.6 |
| Kharchenko et al. | 2016 | 353.887 | 52.682 | â | â | â | â |
| Dias et al. | 2014 | 354.083 | 52.543 | â | -1.65 | -0.32 | â |
| Kharchenko et al. | 2013 | 353.895 | 52.685 | â | 7.55 | -2.0 | -18.6 |
| Kharchenko et al. | 2012 | 353.895 | 52.685 | â | 7.55 | -2.07 | â |
| Piskunov et al. | 2008 | 353.888 | 52.69 | â | â | â | â |
| Piskunov et al. | 2007 | 353.888 | 52.69 | â | â | â | â |
| Kharchenko et al. | 2005 | 353.89 | 52.69 | â | 7.92 | -1.81 | â |
| Kharchenko et al. | 2003 | 353.94 | 52.62 | â | 7.73 | -1.48 | â |
| Dias et al. | 2002 | 354.083 | 52.543 | â | 7.55 | -2.07 | -18.6 |
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] | Bfr | BSS |
|---|---|---|---|---|---|---|---|---|---|
| Li et al. | 2025 | 0.44 | 0.28 | â | 225 | 0.149 | â | â | â |
| Almeida et al. | 2025 | 0.44 | 0.42 | â | 176 | â | 165 | â | â |
| Alfonso et al. | 2024 | 0.45 | 0.29 | â | 77 | 0.003 | â | â | â |
| Zhang et al. | 2024 | â | â | â | â | -0.080* | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 189* | â | â |
| Cavallo et al. | 2024 | 0.44 | 0.53 | â | 126 | 0.240 | â | â | â |
| Hunt & Reffert | 2023 | 0.42 | 0.21 | 0.75 | 124 | â | â | â | â |
| Cordoni et al. | 2023 | 0.44 | 0.42 | â | 176 | 0.002 | 182 | 0.18 | 0.00 |
| Qin et al. | 2023 | 0.51 | 0.40 | â | 100 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 282 | â | 44 | â | â |
| He et al. | 2022 | â | 0.35 | â | 79 | â | â | â | â |
| Tarricq et al. | 2022 | 0.45 | â | â | 112 | â | â | â | â |
| Dias et al. | 2021 | 0.44 | 0.42 | â | 176 | 0.002 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.45 | 0.29 | â | 112 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.44 | â | â | â | â | â | â | â |
| Liu & Pang | 2019 | â | â | â | 46 | -0.750 | â | â | â |
| Bossini et al. | 2019 | 0.41 | 0.27 | â | 154 | 0.000 | â | â | â |
| Soubiran et al. | 2018 | 0.44 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 0.44 | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 0.51 | 0.19 | â | 251 | â | â | â | â |
| Kharchenko et al. | 2016 | 0.43 | 0.16 | â | 282 | â | â | â | â |
| Kharchenko et al. | 2013 | 0.43 | 0.16 | â | 282 | â | â | â | â |
| Kharchenko et al. | 2012 | 0.43 | 0.16 | â | 282 | â | â | â | â |
| Piskunov et al. | 2008 | 0.40 | 0.16 | â | 282 | â | 41* | â | â |
| Piskunov et al. | 2007 | 0.40 | 0.16 | â | 282 | â | 22 | â | â |
| Kharchenko et al. | 2005 | 0.40 | 0.16 | â | 282 | â | â | â | â |
| Kharchenko et al. | 2003 | 0.48 | 0.46 | â | â | â | â | â | â |
| Dias et al. | 2002 | 0.48 | 0.19 | â | 251 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Almeida et al. (2025)
Mass determination: intermediate fit. Isochrone match: good fit.
Cavallo et al. (2024)
Gold sample.