Stock 12

(OCL 258; MWSC 3743; FoF 2399; OCSN 267)

Click to load Aladin Lite
C3
N_50
r_50
AA 220 28.4
Summary

Stock 12 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.

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
Dias et al. (2002) 354.083 52.543 7.55 -2.07 -18.6
Piskunov et al. (2007) 353.888 52.69
Piskunov et al. (2008) 353.888 52.69
Kharchenko et al. (2012) 353.895 52.685 7.55 -2.0
Loktin & Popova (2017) 354.09 52.543 7.55 -2.07 -18.6
Cantat-Gaudin et al. (2018) 353.923 52.685 2.261 8.527 -1.846
Bica et al. (2019) 354.108 52.522
Soubiran et al. (2018) 353.923 52.685 -4.2
Bossini et al. (2019) 353.923 52.685
Liu & Pang (2019) 354.006 52.72 2.256 8.519 -1.853
Cantat-Gaudin et al. (2020) 353.923 52.685 2.261 8.527 -1.846
Dias et al. (2021) 353.978 52.698 2.257 8.547 -1.857 -3.469
Tarricq et al. (2022) 353.803 52.649 2.269 8.522 -1.869
He et al. (2022) 354.008 52.713 2.28 8.535 -1.883
Qin et al. (2023) 353.99 52.66 2.29 8.53 -1.93 -4.63
Cordoni et al. (2023) 353.978 52.698 2.257 8.547 -1.857
Hunt & Reffert (2023) 353.87 52.623 2.287 8.571 -1.917 -3.151
Cavallo et al. (2024) 353.946 52.634 2.289
Hunt & Reffert (2024) 353.87 52.623 2.287 8.571 -1.917 -3.151
Alfonso et al. (2024) -5.941 52.69 2.27 8.513 -2.006
Almeida et al. (2025) 353.978 52.698
           
UCC 353.892 52.645 2.281 8.556 -1.89 -4.172
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

Explore data in Colab

Fundamental parameters

Reference Values
Dias et al. (2002) E(B-V)=0.06, Dist=480.0, Age=8.4
Piskunov et al. (2007) E(B-V)=0.05, Dist=400, logt=8.45, logM=1.35
Piskunov et al. (2008) E(B-V)=0.05, Dist=400, logt=8.45, logM=1.613, logMA=1.557
Kharchenko et al. (2012) e_bv=0.05, distance=430, log_age=8.45
Loktin & Popova (2017) E(B-V)=0.06, Dist=506, logt=8.4
Cantat-Gaudin et al. (2018) dmode=436.8
Soubiran et al. (2018) dmode=436.8
Bossini et al. (2019) AV=0.27, Dist=8.07, logA=8.188, Fe/H=0.0
Liu & Pang (2019) Age=0.046, Z=-0.75
Cantat-Gaudin et al. (2020) AVNN=0.29, DistPc=454.0, AgeNN=8.05
Dias et al. (2021) Av=0.417, Dist=436, logage=8.245, [Fe/H]=0.002
Tarricq et al. (2022) Dist=448, logAgeNN=8.05
He et al. (2022) A0=0.35, logAge=7.9
Qin et al. (2023) E(B-V)=0.13, m-M=8.55, logt=8.0
Cordoni et al. (2023) Av=0.417, Dist=8.197, logAge=8.245, [Fe/H]=0.002, mass-single=182.11, fbin-tot=0.182, fbss-MS=0.0
Hunt & Reffert (2023) AV50=0.212, diffAV50=0.746, MOD50=8.101, logAge50=8.095
Cavallo et al. (2024) AV50=0.53, dMod50=8.23, logAge50=8.1, [Fe/H]50=0.24
Hunt & Reffert (2024) MassJ=189.032, MassTot=286.594
Alfonso et al. (2024) AV=0.2909, MOD=8.28899, logAge=7.88839, Z=0.00296
Almeida et al. (2025) AV=0.417, Dist=436, logAge=8.245, MassRk=165.1

Search coordinates in Bayestar19

Cluster region map