Stock 2
(MWSC 173; FoF 2408; OCSN 265)
1.0
UTI
1.0
CN
1.0
Cdens
1.0
CC3
1.0
Clit
1.0
Cdup
Radius (P>50% members)
49.4 [arcmin]
- CN 1.0 Very rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
Stock 2 is a very rich, very dense object of very high C3 quality. Its parallax locates it at a very close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a massive, 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
Moderate extinction
Massive
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 | 33.861 | 59.556 | 2.669 | 15.838 | -13.729 | 8.817 |
| Li et al. | 2025 | 33.856 | 59.522 | 2.641 | 15.966 | -13.627 | â |
| Wei et al. | 2025 | 33.892 | 59.542 | 2.662 | 15.811 | -13.729 | â |
| Almeida et al. | 2025 | 33.853 | 59.537 | â | â | â | â |
| Alfonso et al. | 2024 | 33.865 | 59.523 | 2.645 | 15.824 | -13.754 | â |
| Zhang et al. | 2024 | 33.85 | 59.577 | â | â | â | â |
| Hunt & Reffert | 2024 | 33.85 | 59.577 | 2.675 | 15.829 | -13.713 | 8.168 |
| Cavallo et al. | 2024 | 33.768 | 59.545 | 2.671 | â | â | â |
| Hunt & Reffert | 2023 | 33.85 | 59.577 | 2.675 | 15.829 | -13.713 | 8.168 |
| Qin et al. | 2023 | 33.88 | 59.52 | 2.68 | 15.82 | -13.78 | 8.57 |
| Just et al. | 2023 | 33.648 | 59.438 | â | â | â | â |
| He et al. | 2022 | 33.899 | 59.56 | 2.674 | 15.812 | -13.75 | â |
| Tarricq et al. | 2022 | 33.88 | 59.45 | 2.662 | 15.816 | -13.748 | â |
| Jaehnig et al. | 2021 | 33.813 | 59.542 | 2.665 | 15.886 | -13.599 | â |
| Rain et al. | 2021 | 33.856 | 59.522 | 2.641 | 15.966 | -13.627 | â |
| Dias et al. | 2021 | 33.853 | 59.537 | 2.641 | 15.845 | -13.698 | 8.757 |
| Cantat-Gaudin et al. | 2020 | 33.856 | 59.522 | 2.641 | 15.966 | -13.627 | â |
| Cantat-Gaudin & Anders | 2020 | 33.856 | 59.522 | 2.641 | 15.966 | -13.627 | â |
| Liu & Pang | 2019 | 33.832 | 59.562 | 2.638 | 15.841 | -13.673 | â |
| Soubiran et al. | 2018 | 33.856 | 59.522 | â | â | â | 8.19 |
| Cantat-Gaudin et al. | 2018 | 33.856 | 59.522 | 2.641 | 15.966 | -13.627 | â |
| Loktin & Popova | 2017 | 33.675 | 59.485 | â | 1.744 | -1.948 | 1.8 |
| Kharchenko et al. | 2016 | 33.648 | 59.438 | â | â | â | â |
| Dias et al. | 2014 | 33.679 | 59.485 | â | -0.24 | -0.51 | â |
| Kharchenko et al. | 2013 | 33.66 | 59.44 | â | 16.13 | -14.5 | 1.8 |
| Gozha et al. | 2012 | 33.679 | 59.485 | â | â | â | â |
| Kharchenko et al. | 2012 | 33.66 | 59.44 | â | 16.13 | -14.5 | 1.81 |
| Piskunov et al. | 2008 | 33.588 | 59.263 | â | â | â | â |
| Kharchenko et al. | 2007 | 33.67 | 59.49 | â | 2.8 | â | -2.85 |
| Piskunov et al. | 2007 | 33.588 | 59.263 | â | â | â | â |
| van den Bergh | 2006 | 33.6 | 59.267 | â | â | â | â |
| Kharchenko et al. | 2005 | 33.6 | 59.27 | â | 16.22 | -13.39 | -2.85 |
| Kharchenko et al. | 2003 | 33.69 | 59.39 | â | 16.49 | -13.16 | â |
| Dias et al. | 2002 | 33.679 | 59.485 | â | 17.29 | -13.1 | -41.14 |
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 | 0.37 | 0.81 | â | 606 | 0.054 | â | â | â |
| Wei et al. | 2025 | 0.42 | 1.01 | â | 245 | 0.250 | 1520 | 0.59 | â |
| Almeida et al. | 2025 | 0.37 | 0.79 | â | 804 | â | 1753 | â | â |
| Alfonso et al. | 2024 | 0.40 | 0.50 | â | 1094 | 0.032 | â | â | â |
| Zhang et al. | 2024 | â | â | â | â | -0.081* | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 3319* | â | â |
| Cavallo et al. | 2024 | 0.38 | 1.23 | â | 234 | 0.290 | â | â | â |
| Hunt & Reffert | 2023 | 0.36 | 0.90 | 2.02 | 290 | â | â | â | â |
| Qin et al. | 2023 | 0.50 | 0.78 | â | 355 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 275 | â | 2075 | â | â |
| He et al. | 2022 | â | 1.30 | â | 282 | â | â | â | â |
| Tarricq et al. | 2022 | 0.43 | â | â | 398 | â | â | â | â |
| Jaehnig et al. | 2021 | 0.38* | â | â | â | â | â | â | â |
| Rain et al. | 2021 | 0.37 | 1.18 | â | 170 | â | â | â | 0 |
| Dias et al. | 2021 | 0.37 | 0.79 | â | 804 | 0.029 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.40 | 0.50 | â | 398 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.37 | â | â | â | â | â | â | â |
| Liu & Pang | 2019 | â | â | â | 676 | 0.250 | â | â | â |
| Soubiran et al. | 2018 | 0.37 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 0.37 | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 0.39 | 1.04 | â | 164 | â | â | â | â |
| Kharchenko et al. | 2016 | 0.40 | 1.05 | â | 275 | â | â | â | â |
| Kharchenko et al. | 2013 | 0.40 | 1.05 | â | 275 | -0.140 | â | â | â |
| Gozha et al. | 2012 | 0.30 | â | â | 170 | -0.140 | 9772 | â | â |
| Kharchenko et al. | 2012 | 0.40 | 1.05 | â | 275 | -0.140 | â | â | â |
| Piskunov et al. | 2008 | 0.38 | 1.05 | â | 148 | â | 24155* | â | â |
| Piskunov et al. | 2007 | 0.38 | 1.05 | â | 148 | â | 12677 | â | â |
| van den Bergh | 2006 | 0.30 | 1.18 | â | 170 | â | â | â | â |
| Kharchenko et al. | 2005 | 0.38 | 1.05 | â | 148 | â | â | â | â |
| Kharchenko et al. | 2003 | 0.30 | 1.18 | â | â | â | â | â | â |
| Dias et al. | 2002 | 0.30 | 1.18 | â | 170 | -0.140 | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


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