NGC 5269

(ESO 097 04; MWSC 2156; FoF 261)

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C3
N_50
r_50
AA 218 3.9
Summary

NGC 5269 is a rich, very dense object of very high C3 quality. It is located at a moderate distance from the Sun, near the mid-plane. It is well-studied in the literature.

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

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
Dias et al. (2002) 206.183 -62.915 -1.68 -6.25
Kharchenko et al. (2012) 206.183 -62.892 -7.03 -1.19
Cantat-Gaudin et al. (2018) 206.147 -62.907 0.46 -4.49 -1.918
Bica et al. (2019) 206.194 -62.916
Soubiran et al. (2018) 206.147 -62.907 -36.91
Liu & Pang (2019) 206.119 -62.919 0.471 -4.574 -1.936
Cantat-Gaudin et al. (2020) 206.147 -62.907 0.46 -4.49 -1.918
Dias et al. (2021) 206.159 -62.906 0.463 -4.498 -1.921 -37.259
Hunt & Reffert (2023) 206.167 -62.906 0.481 -4.541 -1.898 -37.778
Cavallo et al. (2024) 206.177 -62.906 0.483
Hunt & Reffert (2024) 206.167 -62.906 0.481 -4.541 -1.898 -37.778
Almeida et al. (2025) 206.159 -62.906
           
UCC 206.16 -62.91 0.486 -4.536 -1.898 -34.654
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)=0.52, Dist=1410.0, Age=8.2
Kharchenko et al. (2012) e_bv=0.416, distance=1634, log_age=8.52
Cantat-Gaudin et al. (2018) dmode=2044.6
Soubiran et al. (2018) dmode=2044.6
Liu & Pang (2019) Age=0.174, Z=0.0
Cantat-Gaudin et al. (2020) AVNN=0.99, DistPc=2080.0, AgeNN=8.12
Dias et al. (2021) Av=1.437, Dist=1805, logage=8.095, [Fe/H]=0.153
Hunt & Reffert (2023) AV50=1.289, diffAV50=2.028, MOD50=11.409, logAge50=8.349
Cavallo et al. (2024) AV50=1.63, dMod50=11.07, logAge50=8.58, [Fe/H]50=-0.36
Hunt & Reffert (2024) MassJ=1143.11, MassTot=1143.11
Almeida et al. (2025) AV=1.437, Dist=1805, logAge=8.095, MassRk=334.1

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
SAI 118 0.5 205.81 -63.14 0.53 -4.47 -2.3 -15.08 0.9