Stock 8
(FSR 0780; BDS2003 69)
0.91
UTI
0.81
CN
1.0
Cdens
0.75
CC3
1.0
Clit
1.0
Cdup
Stellar density (N50/rad)
16.2 [N/pc2]
- CN 0.81 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
Stock 8 is a rich, very dense object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a massive, near-solar metallicity, very young 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.
Note: This object shares a small percentage of members with 3 later reported entries. 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 | 81.959 | 34.428 | 0.462 | 0.085 | -2.343 | -59.372 |
| Almeida et al. | 2025 | 81.959 | 34.496 | â | â | â | â |
| Zhang et al. | 2024 | 82.029 | 34.421 | â | â | â | â |
| Hunt & Reffert | 2024 | 82.029 | 34.421 | 0.47 | 0.034 | -2.348 | -51.155 |
| Celli et al. | 2024 | 81.956 | 34.452 | â | â | â | â |
| Cavallo et al. | 2024 | 81.951 | 34.548 | 0.47 | â | â | â |
| Hunt & Reffert | 2023 | 82.029 | 34.421 | 0.47 | 0.034 | -2.348 | -51.155 |
| Jaehnig et al. | 2021 | 81.959 | 34.46 | 0.48 | 0.106 | -2.272 | â |
| Rain et al. | 2021 | 81.956 | 34.452 | 0.446 | 0.094 | -2.249 | â |
| Dias et al. | 2021 | 81.959 | 34.496 | 0.447 | 0.1 | -2.252 | â |
| Cantat-Gaudin et al. | 2020 | 81.956 | 34.452 | 0.446 | 0.094 | -2.249 | â |
| Cantat-Gaudin & Anders | 2020 | 81.956 | 34.452 | 0.446 | 0.094 | -2.249 | â |
| Cantat-Gaudin et al. | 2018 | 81.956 | 34.452 | 0.446 | 0.094 | -2.249 | â |
| Loktin & Popova | 2017 | 82.035 | 34.423 | â | 0.592 | -1.905 | -6.4 |
| Dias et al. | 2014 | 82.029 | 34.423 | â | -1.07 | -3.02 | â |
| Gozha et al. | 2012 | 82.029 | 34.423 | â | â | â | â |
| Glushkova et al. | 2010 | 82.037 | 34.431 | â | â | â | â |
| Piskunov et al. | 2008 | 82.026 | 34.425 | â | â | â | â |
| Kharchenko et al. | 2007 | 82.03 | 34.42 | â | 0.25 | â | -6.4 |
| Froebrich et al. | 2007 | 81.858 | 34.403 | â | â | â | â |
| van den Bergh | 2006 | 82.05 | 34.417 | â | â | â | â |
| Kharchenko et al. | 2005 | 82.03 | 34.42 | â | -1.44 | -3.9 | -6.4 |
| Kharchenko et al. | 2003 | 81.88 | 34.43 | â | -1.44 | -4.35 | â |
| Dias et al. | 2002 | 82.029 | 34.423 | â | -1.07 | -3.02 | -18.01 |
| Dambis | 1999 | 82.031 | 34.428 | 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 | 2.0 | 1.365 | 2.26 | 10 | -0.071 | 2008 | â | 0.0 |
| Almeida et al. | 2025 | 2.03 | 1.69 | â | 10 | â | 2105 | â | â |
| Zhang et al. | 2024 | â | â | â | â | -0.060(1) | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 2065(1) | â | â |
| Celli et al. | 2024 | â | â | â | 14 | â | 1779 | â | â |
| Cavallo et al. | 2024 | 1.79 | 1.70 | â | 6 | -0.420 | â | â | â |
| Hunt & Reffert | 2023 | 1.96 | 1.76 | 2.26 | 10 | â | â | â | â |
| Jaehnig et al. | 2021 | 2.06(1) | â | â | â | â | â | â | â |
| Rain et al. | 2021 | 2.11 | 1.24 | â | 2 | â | â | â | 0 |
| Dias et al. | 2021 | 2.03 | 1.69 | â | 10 | -0.071 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 2.36 | 1.17 | â | 14 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 2.11 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 2.11 | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 1.80 | 1.37 | â | 12 | â | â | â | â |
| Gozha et al. | 2012 | 2.00 | â | â | 2 | â | 1950 | â | â |
| Glushkova et al. | 2010 | 0.90 | 3.75 | â | 32 | â | â | â | â |
| Piskunov et al. | 2008 | 1.82 | 1.36 | â | 41 | â | â | â | â |
| van den Bergh | 2006 | 1.82 | 1.36 | â | 11 | â | â | â | â |
| Kharchenko et al. | 2005 | 1.82 | 1.36 | â | 41 | â | â | â | â |
| Kharchenko et al. | 2003 | 1.82 | 1.36 | â | â | â | â | â | â |
| Dias et al. | 2002 | 2.00 | 1.24 | â | 2 | â | â | â | â |
| Dambis | 1999 | 2.15 | 1.41 | â | 10 | 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: intermediate fit. Isochrone match: good fit.
Cavallo et al. (2024)
Gold sample.