NGC 136

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C3
N_50
r_50
AB 156 1.8
Summary

NGC 136 is a rich, very dense object of high C3 quality. It is located at a large distance from the Sun, below the mid-plane. It is very well-studied in the literature.

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Positions

Reference RA DEC Plx pmRA pmDE Rv
Dias et al. (2002) 7.888 61.508 -0.38 1.21
Kharchenko et al. (2012) 7.901 61.51 0.31 -1.16
Loktin & Popova (2017) 7.89 61.508 -0.806 -0.785
Cantat-Gaudin et al. (2018) 7.896 61.506 0.181 -1.648 -0.522
Soubiran et al. (2018) 7.896 61.506 -47.38
Donor et al. (2020) 7.901 61.51 -1.63 -0.53 -51.9
Cantat-Gaudin et al. (2020) 7.896 61.506 0.181 -1.648 -0.522
Dias et al. (2021) 7.893 61.507 0.18 -1.633 -0.517
Rain et al. (2021) 7.896 61.506 0.181 -1.648 -0.522
Jaehnig et al. (2021) 7.891 61.505 0.2 -1.633 -0.529
Hunt & Reffert (2023) 7.891 61.508 0.201 -1.637 -0.576 -56.218
Cavallo et al. (2024) 7.88 61.507 0.2
Hunt & Reffert (2024) 7.891 61.508 0.201 -1.637 -0.576 -56.218
Almeida et al. (2025) 7.893 61.507
           
UCC 7.891 61.507 0.198 -1.623 -0.585 -52.677
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

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Estimated members

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Fundamental parameters

Reference Values
Dias et al. (2002) E(B-V)=0.7, Dist=5220.0, Age=8.4, [Fe/H]=-0.05
Kharchenko et al. (2012) e_bv=0.833, distance=3519, log_age=8.4
Loktin & Popova (2017) E(B-V)=0.398, Dist=3054, logt=8.42
Cantat-Gaudin et al. (2018) dmode=4767.3
Soubiran et al. (2018) dmode=4767.3
Donor et al. (2020) Fe/H=-0.23
Cantat-Gaudin et al. (2020) AVNN=1.76, DistPc=5141.0, AgeNN=8.41
Dias et al. (2021) Av=2.128, Dist=4156, logage=8.405, [Fe/H]=-0.216
Rain et al. (2021) E(B-V)=0.7, Dist=4767.3, log(Age)=8.4, NBSS=0
Jaehnig et al. (2021) dmode=5.035
Hunt & Reffert (2023) AV50=1.944, diffAV50=1.663, MOD50=13.332, logAge50=8.558
Cavallo et al. (2024) AV50=1.84, dMod50=13.04, logAge50=8.65, [Fe/H]50=0.15
Hunt & Reffert (2024) MassJ=1323.07, MassTot=1446.74
Almeida et al. (2025) AV=2.128, Dist=4156, logAge=8.405, MassRk=550.1

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Cluster region map