NGC 2169

(FSR 0947; MWSC 740)

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C3
N_50
r_50
AB 149 6.1
Summary

NGC 2169 is a rich, very dense object of high C3 quality. It is located at a close distance from the Sun, near the mid-plane. It is very well-studied in the literature.

This object shares a large percentage of members with a later reported entry.

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
Dambis (1999) 92.125 13.967
Dias et al. (2002) 92.1 13.965 -4.21 -2.45 22.5
Chen et al. (2003) 92.127 13.988 -4.21 -2.45 17.0
Kharchenko et al. (2003) 92.13 13.97 -2.96 -3.74
Kharchenko et al. (2005) 92.1 13.97 -2.17 -2.52 22.22
Froebrich et al. (2007) 92.246 13.876
Kharchenko et al. (2007) 92.1 13.97 0.15 22.23
Piskunov et al. (2008) 92.091 13.969
Kharchenko et al. (2013) 92.1 13.99 -1.84 -2.37 22.3
Kharchenko et al. (2016) 92.092 13.991
Loktin & Popova (2017) 92.1 13.966 0.072 -0.856 22.3
Cantat-Gaudin et al. (2020) 92.125 13.951 0.982 -1.068 -1.655
Dias et al. (2021) 92.129 13.937 0.975 -1.059 -1.659
Rain et al. (2021) 92.125 13.951 0.982 -1.068 -1.655
Jaehnig et al. (2021) 92.122 13.951 1.048 -1.076 -1.661
He et al. (2022) 92.129 13.962 1.038 -1.127 -1.613
Just et al. (2023) 92.092 13.991
Hunt & Reffert (2023) 92.118 13.967 1.035 -1.086 -1.612 17.224
Cavallo et al. (2024) 92.144 13.918 1.033
Celli et al. (2024) 92.125 13.951
Hunt & Reffert (2024) 92.118 13.967 1.035 -1.086 -1.612 17.224
Zhang et al. (2024) 92.118 13.967
Almeida et al. (2025) 92.129 13.937
           
UCC 92.127 13.947 1.038 -1.096 -1.604 10.488
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
Dambis (1999) E_B-V_=0.193, DM0=9.98, log_age_=7.0
Dias et al. (2002) E(B-V)=0.199, Dist=1052.0, Age=7.067
Chen et al. (2003) HDis=1052, Age=0.01
Kharchenko et al. (2003) E(B-V)=0.2, Dist=1052
Kharchenko et al. (2005) E(B-V)=0.2, Dist=1032, logt=6.89
Piskunov et al. (2008) E(B-V)=0.2, Dist=1032, logt=6.89, logMA=1.481
Kharchenko et al. (2013) E(B-V)=0.2, d=1032.0, logt=6.89
Kharchenko et al. (2016) E(B-V)=0.2, d=1032.0, logt=6.89
Loktin & Popova (2017) E(B-V)=0.2, Dist=1045, logt=7.062
Cantat-Gaudin et al. (2020) AVNN=0.85, DistPc=1072.0, AgeNN=7.09
Dias et al. (2021) Av=0.819, Dist=1004, logage=6.89, [Fe/H]=-0.092
Rain et al. (2021) E(B-V)=0.19, Dist=989.5, log(Age)=7.06, NBSS=0
Jaehnig et al. (2021) dmode=0.94
He et al. (2022) A0=0.8, logAge=6.8
Just et al. (2023) logt=6.89, logmt=1.612
Hunt & Reffert (2023) AV50=0.58, diffAV50=1.21, MOD50=9.838, logAge50=6.723
Cavallo et al. (2024) AV50=0.78, dMod50=9.85, logAge50=6.52, [Fe/H]50=-0.06
Celli et al. (2024) Age=12.3, Mc=198.9
Hunt & Reffert (2024) MassJ=230.174, MassTot=232.696
Zhang et al. (2024) [Fe/H]ANN=-0.2241, [Fe/H]MCMC=-0.2040
Almeida et al. (2025) AV=0.819, Dist=1004, logAge=6.89, MassRk=169.4

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
OC 0323 75.8 92.13 13.95 1.04 -1.1 -1.6 8.95 0.0