Stock 8

(FSR 0780; BDS2003 69)

Click to load Aladin Lite
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

â„šī¸
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.

Almeida et al. (2025)
Mass determination: intermediate fit. Isochrone match: good fit.

Cavallo et al. (2024)
Gold sample.

Data

â„šī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 81.959 34.428 0.462 0.085 -2.343 -59.372
Almeida et al. 2025 81.959 34.496 – – – –
Zhang et al. 2024 82.029 34.421 – – – –
Hunt & Reffert 2024 82.029 34.421 0.47 0.034 -2.348 -51.155
Celli et al. 2024 81.956 34.452 – – – –
Cavallo et al. 2024 81.951 34.548 0.47 – – –
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 –
Rain et al. 2021 81.956 34.452 0.446 0.094 -2.249 –
Dias et al. 2021 81.959 34.496 0.447 0.1 -2.252 –
Cantat-Gaudin et al. 2020 81.956 34.452 0.446 0.094 -2.249 –
Cantat-Gaudin & Anders 2020 81.956 34.452 0.446 0.094 -2.249 –
Cantat-Gaudin et al. 2018 81.956 34.452 0.446 0.094 -2.249 –
Loktin & Popova 2017 82.035 34.423 – 0.592 -1.905 -6.4
Dias et al. 2014 82.029 34.423 – -1.07 -3.02 –
Gozha et al. 2012 82.029 34.423 – – – –
Glushkova et al. 2010 82.037 34.431 – – – –
Piskunov et al. 2008 82.026 34.425 – – – –
Kharchenko et al. 2007 82.03 34.42 – 0.25 – -6.4
Froebrich et al. 2007 81.858 34.403 – – – –
van den Bergh 2006 82.05 34.417 – – – –
Kharchenko et al. 2005 82.03 34.42 – -1.44 -3.9 -6.4
Kharchenko et al. 2003 81.88 34.43 – -1.44 -4.35 –
Dias et al. 2002 82.029 34.423 – -1.07 -3.02 -18.01
Dambis 1999 82.031 34.428 – – – –

💡 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 99999– 2.0 1.365 2.26 10 -0.071 2008 – 0.0
Almeida et al. 2025 2.03 1.69 – 10 – 2105 – –
Zhang et al. 2024 – – – – -0.060(1) – – –
Hunt & Reffert 2024 – – – – – 2065(1) – –
Celli et al. 2024 – – – 14 – 1779 – –
Cavallo et al. 2024 1.79 1.70 – 6 -0.420 – – –
Hunt & Reffert 2023 1.96 1.76 2.26 10 – – – –
Jaehnig et al. 2021 2.06(1) – – – – – – –
Rain et al. 2021 2.11 1.24 – 2 – – – 0
Dias et al. 2021 2.03 1.69 – 10 -0.071 – – –
Cantat-Gaudin et al. 2020 2.36 1.17 – 14 – – – –
Cantat-Gaudin & Anders 2020 2.11 – – – – – – –
Cantat-Gaudin et al. 2018 2.11 – – – – – – –
Loktin & Popova 2017 1.80 1.37 – 12 – – – –
Gozha et al. 2012 2.00 – – 2 – 1950 – –
Glushkova et al. 2010 0.90 3.75 – 32 – – – –
Piskunov et al. 2008 1.82 1.36 – 41 – – – –
van den Bergh 2006 1.82 1.36 – 11 – – – –
Kharchenko et al. 2005 1.82 1.36 – 41 – – – –
Kharchenko et al. 2003 1.82 1.36 – – – – – –
Dias et al. 2002 2.00 1.24 – 2 – – – –
Dambis 1999 2.15 1.41 – 10 – – – –

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Cluster % RA DEC Plx pmRA pmDE Rv UTI
HSC 1356 11.8 81.86 34.39 0.46 0.17 -1.87 79.39 0.08
FSR 0777 2.0 81.9 34.75 0.47 -0.01 -2.29 – 0.46
Kronberger 1 0.4 82.04 34.78 0.46 -0.04 -2.23 – 0.64

💡 Note: The % column shows the percentage of members that Stock 8 shares with each listed object.

Visualization

â„šī¸