Stock 10
(MWSC 616; OCSN 266)
0.97
UTI
0.86
CN
1.0
Cdens
1.0
CC3
1.0
Clit
1.0
Cdup
Radius (P>50% members)
41.5 [arcmin]
- CN 0.86 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
Stock 10 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 low-mass, near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the age parameter (see Parameters). It is very well-studied in the literature.
Very close
Low extinction
Low mass
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 | 84.85 | 37.808 | 2.785 | -3.139 | -0.429 | -13.534 |
| Li et al. | 2025 | 84.808 | 37.85 | 2.759 | -3.114 | -0.464 | â |
| Almeida et al. | 2025 | 84.835 | 37.86 | â | â | â | â |
| Alfonso et al. | 2024 | 84.841 | 37.793 | 2.759 | -3.153 | -0.424 | â |
| Zhang et al. | 2024 | 84.742 | 37.808 | â | â | â | â |
| Hunt & Reffert | 2024 | 84.742 | 37.808 | 2.794 | -3.15 | -0.428 | -12.7 |
| Cavallo et al. | 2024 | 84.907 | 37.75 | 2.8 | â | â | â |
| Hunt & Reffert | 2023 | 84.742 | 37.808 | 2.794 | -3.15 | -0.428 | -12.7 |
| Almeida et al. | 2023 | 84.938 | 37.882 | â | â | â | â |
| Qin et al. | 2023 | 84.88 | 37.78 | 2.8 | -3.16 | -0.43 | -13.58 |
| Just et al. | 2023 | 84.8 | 37.805 | â | â | â | â |
| He et al. | 2022 | 84.855 | 37.854 | 2.795 | -3.155 | -0.417 | â |
| Tarricq et al. | 2022 | 84.693 | 37.692 | 2.789 | -3.155 | -0.417 | â |
| Dias et al. | 2021 | 84.835 | 37.86 | 2.748 | -3.153 | -0.476 | -12.592 |
| Cantat-Gaudin et al. | 2020 | 84.808 | 37.85 | 2.759 | -3.114 | -0.464 | â |
| Cantat-Gaudin & Anders | 2020 | 84.808 | 37.85 | 2.759 | -3.114 | -0.464 | â |
| Bossini et al. | 2019 | 84.808 | 37.85 | â | â | â | â |
| Soubiran et al. | 2018 | 84.808 | 37.85 | â | â | â | -11.67 |
| Cantat-Gaudin et al. | 2018 | 84.808 | 37.85 | 2.759 | -3.114 | -0.464 | â |
| Loktin & Popova | 2017 | 84.75 | 37.934 | â | -1.49 | -4.44 | -8.16 |
| Kharchenko et al. | 2016 | 84.8 | 37.805 | â | â | â | â |
| Dias et al. | 2014 | 84.75 | 37.933 | â | -1.49 | -4.44 | â |
| Kharchenko et al. | 2013 | 84.81 | 37.805 | â | -1.18 | -2.0 | -8.2 |
| Gozha et al. | 2012 | 84.75 | 37.933 | â | â | â | â |
| Kharchenko et al. | 2012 | 84.81 | 37.805 | â | -1.18 | -2.0 | -8.16 |
| Piskunov et al. | 2008 | 84.739 | 37.926 | â | â | â | â |
| Kharchenko et al. | 2007 | 84.75 | 37.93 | â | 0.32 | â | -8.66 |
| Piskunov et al. | 2007 | 84.739 | 37.926 | â | â | â | â |
| van den Bergh | 2006 | 84.75 | 37.933 | â | â | â | â |
| Kharchenko et al. | 2005 | 84.75 | 37.93 | â | -3.34 | -1.57 | -8.15 |
| Kharchenko et al. | 2003 | 84.67 | 37.81 | â | -2.48 | -3.66 | â |
| Dias et al. | 2002 | 84.75 | 37.933 | â | -1.49 | -4.44 | -8.16 |
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 | 0.36 | 0.54 | â | 96 | -0.042 | â | â | â |
| Almeida et al. | 2025 | 0.36 | 0.47 | â | 233 | â | 205 | â | â |
| Alfonso et al. | 2024 | 0.37 | 0.44 | â | 84 | -0.004 | â | â | â |
| Zhang et al. | 2024 | â | â | â | â | -0.087* | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 329* | â | â |
| Cavallo et al. | 2024 | 0.37 | 0.77 | â | 74 | 0.000 | â | â | â |
| Hunt & Reffert | 2023 | 0.34 | 0.29 | 0.89 | 135 | â | â | â | â |
| Almeida et al. | 2023 | 0.35 | 0.68 | â | 136 | -0.120 | 194* | 0.42 | â |
| Qin et al. | 2023 | 0.42 | 0.50 | â | 89 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 263 | â | 38 | â | â |
| He et al. | 2022 | â | 0.50 | â | 79 | â | â | â | â |
| Tarricq et al. | 2022 | 0.37 | â | â | 83 | â | â | â | â |
| Dias et al. | 2021 | 0.36 | 0.47 | â | 233 | -0.004 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 0.37 | 0.44 | â | 81 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 0.36 | â | â | â | â | â | â | â |
| Bossini et al. | 2019 | 0.33 | 0.26 | â | 115 | 0.000 | â | â | â |
| Soubiran et al. | 2018 | 0.36 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 0.36 | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 0.38 | 0.22 | â | 79 | â | â | â | â |
| Kharchenko et al. | 2016 | 0.50 | 0.24 | â | 263 | â | â | â | â |
| Kharchenko et al. | 2013 | 0.50 | 0.24 | â | 263 | â | â | â | â |
| Gozha et al. | 2012 | 0.38 | â | â | 79 | â | 42 | â | â |
| Kharchenko et al. | 2012 | 0.50 | 0.24 | â | 263 | â | â | â | â |
| Piskunov et al. | 2008 | 0.38 | 0.25 | â | 263 | â | 42* | â | â |
| Piskunov et al. | 2007 | 0.38 | 0.25 | â | 263 | â | 13 | â | â |
| van den Bergh | 2006 | 0.38 | 0.19 | â | 224 | â | â | â | â |
| Kharchenko et al. | 2005 | 0.38 | 0.25 | â | 263 | â | â | â | â |
| Kharchenko et al. | 2003 | 0.67 | 0.62 | â | â | â | â | â | â |
| Dias et al. | 2002 | 0.38 | 0.22 | â | 79 | â | 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. Silver sample.
Cavallo et al. (2024)
Gold sample.