Stock 10
(OCSN 266)
Summary
Stock 10 is a rich, very dense object of very high C3 quality. It is located at a very close distance from the Sun, near the mid-plane. It is very well-studied in the literature.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| Dias et al. (2002) | 84.75 | 37.933 | – | -1.49 | -4.44 | -8.16 |
| Piskunov et al. (2007) | 84.739 | 37.926 | – | – | – | – |
| Piskunov et al. (2008) | 84.739 | 37.926 | – | – | – | – |
| Kharchenko et al. (2012) | 84.81 | 37.805 | – | -1.18 | -2.0 | – |
| Loktin & Popova (2017) | 84.75 | 37.934 | – | -1.49 | -4.44 | -8.16 |
| Cantat-Gaudin et al. (2018) | 84.808 | 37.85 | 2.759 | -3.114 | -0.464 | – |
| Soubiran et al. (2018) | 84.808 | 37.85 | – | – | – | -11.67 |
| Bossini et al. (2019) | 84.808 | 37.85 | – | – | – | – |
| Cantat-Gaudin et al. (2020) | 84.808 | 37.85 | 2.759 | -3.114 | -0.464 | – |
| Dias et al. (2021) | 84.835 | 37.86 | 2.748 | -3.153 | -0.476 | -12.592 |
| Tarricq et al. (2022) | 84.693 | 37.692 | 2.789 | -3.155 | -0.417 | – |
| He et al. (2022) | 84.855 | 37.854 | 2.795 | -3.155 | -0.417 | – |
| Qin et al. (2023) | 84.88 | 37.78 | 2.8 | -3.16 | -0.43 | -13.58 |
| Hunt & Reffert (2023) | 84.742 | 37.808 | 2.794 | -3.15 | -0.428 | -12.7 |
| Cavallo et al. (2024) | 84.907 | 37.75 | 2.8 | – | – | – |
| Hunt & Reffert (2024) | 84.742 | 37.808 | 2.794 | -3.15 | -0.428 | -12.7 |
| Alfonso et al. (2024) | 84.841 | 37.793 | 2.759 | -3.153 | -0.424 | – |
| Almeida et al. (2025) | 84.835 | 37.86 | – | – | – | – |
| UCC | 84.85 | 37.808 | 2.785 | -3.139 | -0.429 | -13.534 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Dias et al. (2002) | E(B-V)=0.07, Dist=380.0, Age=7.9 |
| Piskunov et al. (2007) | E(B-V)=0.08, Dist=380, logt=8.42, logM=1.127 |
| Piskunov et al. (2008) | E(B-V)=0.08, Dist=380, logt=8.42, logM=1.622, logMA=1.622 |
| Kharchenko et al. (2012) | e_bv=0.079, distance=500, log_age=8.42 |
| Loktin & Popova (2017) | E(B-V)=0.07, Dist=382, logt=7.9 |
| Cantat-Gaudin et al. (2018) | dmode=358.7 |
| Soubiran et al. (2018) | dmode=358.7 |
| Bossini et al. (2019) | AV=0.255, Dist=7.574, logA=8.06, Fe/H=0.0 |
| Cantat-Gaudin et al. (2020) | AVNN=0.44, DistPc=373.0, AgeNN=7.91 |
| Dias et al. (2021) | Av=0.467, Dist=359, logage=8.367, [Fe/H]=-0.004 |
| Tarricq et al. (2022) | Dist=369, logAgeNN=7.92 |
| He et al. (2022) | A0=0.5, logAge=7.9 |
| Qin et al. (2023) | E(B-V)=0.16, m-M=8.11, logt=7.95 |
| Hunt & Reffert (2023) | AV50=0.286, diffAV50=0.888, MOD50=7.669, logAge50=8.129 |
| Cavallo et al. (2024) | AV50=0.77, dMod50=7.82, logAge50=7.87, [Fe/H]50=0.0 |
| Hunt & Reffert (2024) | MassJ=328.581, MassTot=382.156 |
| Alfonso et al. (2024) | AV=0.43927, MOD=7.86012, logAge=7.92451, Z=-0.0043 |
| Almeida et al. (2025) | AV=0.467, Dist=359, logAge=8.367, MassRk=204.8 |
Search coordinates in Bayestar19