Stock 2

(FoF 2408; OCSN 265)

Click to load Aladin Lite
C3
N_50
r_50
AA 2019 49.4
Summary

Stock 2 is a very 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) 33.679 59.485 17.29 -13.1 -41.14
Piskunov et al. (2007) 33.588 59.263
Piskunov et al. (2008) 33.588 59.263
Kharchenko et al. (2012) 33.66 59.44 16.13 -14.5
Loktin & Popova (2017) 33.675 59.485 1.744 -1.948 1.8
Cantat-Gaudin et al. (2018) 33.856 59.522 2.641 15.966 -13.627
Soubiran et al. (2018) 33.856 59.522 8.19
Liu & Pang (2019) 33.832 59.562 2.638 15.841 -13.673
Cantat-Gaudin et al. (2020) 33.856 59.522 2.641 15.966 -13.627
Dias et al. (2021) 33.853 59.537 2.641 15.845 -13.698 8.757
Rain et al. (2021) 33.856 59.522 2.641 15.966 -13.627
Jaehnig et al. (2021) 33.813 59.542 2.665 15.886 -13.599
Tarricq et al. (2022) 33.88 59.45 2.662 15.816 -13.748
He et al. (2022) 33.899 59.56 2.674 15.812 -13.75
Qin et al. (2023) 33.88 59.52 2.68 15.82 -13.78 8.57
Hunt & Reffert (2023) 33.85 59.577 2.675 15.829 -13.713 8.168
Cavallo et al. (2024) 33.768 59.545 2.671
Hunt & Reffert (2024) 33.85 59.577 2.675 15.829 -13.713 8.168
Alfonso et al. (2024) 33.865 59.523 2.645 15.824 -13.754
Almeida et al. (2025) 33.853 59.537
           
UCC 33.861 59.556 2.669 15.838 -13.729 8.817
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)=0.38, Dist=303.0, Age=8.23, [Fe/H]=-0.14
Piskunov et al. (2007) E(B-V)=0.34, Dist=380, logt=8.17, logM=4.103
Piskunov et al. (2008) E(B-V)=0.34, Dist=380, logt=8.17, logM=4.383, logMA=3.987
Kharchenko et al. (2012) e_bv=0.339, distance=400, log_age=8.44, metallicity=-0.14
Loktin & Popova (2017) E(B-V)=0.334, Dist=392, logt=8.214
Cantat-Gaudin et al. (2018) dmode=374.5
Soubiran et al. (2018) dmode=374.5
Liu & Pang (2019) Age=0.676, Z=0.25
Cantat-Gaudin et al. (2020) AVNN=0.5, DistPc=399.0, AgeNN=8.6
Dias et al. (2021) Av=0.791, Dist=374, logage=8.905, [Fe/H]=0.029
Rain et al. (2021) E(B-V)=0.38, Dist=374.5, log(Age)=8.23, NBSS=0
Jaehnig et al. (2021) dmode=0.375
Tarricq et al. (2022) Dist=435, logAgeNN=8.6
He et al. (2022) A0=1.3, logAge=8.45
Qin et al. (2023) E(B-V)=0.25, m-M=8.48, logt=8.55
Hunt & Reffert (2023) AV50=0.9, diffAV50=2.019, MOD50=7.767, logAge50=8.463
Cavallo et al. (2024) AV50=1.23, dMod50=7.92, logAge50=8.37, [Fe/H]50=0.29
Hunt & Reffert (2024) MassJ=3318.85, MassTot=3764.31
Alfonso et al. (2024) AV=0.49866, MOD=8.00463, logAge=9.03889, Z=0.03198
Almeida et al. (2025) AV=0.791, Dist=374, logAge=8.905, MassRk=1753.0

Search coordinates in Bayestar19

Cluster region map