Collinder 149

(NGC 2401; MWSC 1241; OCL 588)

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C3
N_50
r_50
AA 157 2.0
Summary

Collinder 149 is a rich, very dense object of very high C3 quality. It is located at a moderate distance from the Sun, above 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) 112.35 -13.967 2.01 4.43
Kharchenko et al. (2013) 112.351 -13.972 2.01 4.43
Kharchenko et al. (2016) 112.345 -13.97
Cantat-Gaudin et al. (2018) 112.352 -13.968 0.203 -1.37 1.673
Bica et al. (2019) 112.344 -13.964
Cantat-Gaudin et al. (2020) 112.352 -13.968 0.203 -1.37 1.673
Dias et al. (2021) 112.349 -13.966 0.198 -1.367 1.66
Just et al. (2023) 112.345 -13.97
Hunt & Reffert (2023) 112.351 -13.968 0.207 -1.381 1.701
Cavallo et al. (2024) 112.353 -13.965 0.207
Hunt & Reffert (2024) 112.351 -13.968 0.207 -1.381 1.701
Almeida et al. (2025) 112.349 -13.966
           
UCC 112.354 -13.968 0.202 -1.371 1.683 64.103
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)=0.35, Dist=5888.0, Age=7.8
Kharchenko et al. (2013) E(B-V)=0.354, d=3778.0, logt=7.0
Kharchenko et al. (2016) E(B-V)=0.354, d=3778.0, logt=7.0
Cantat-Gaudin et al. (2018) dmode=4300.5
Cantat-Gaudin et al. (2020) AVNN=0.75, DistPc=4749.0, AgeNN=7.78
Dias et al. (2021) Av=1.044, Dist=3940, logage=8.322, [Fe/H]=-0.168
Just et al. (2023) logt=7.0, logmt=2.71
Hunt & Reffert (2023) AV50=0.885, diffAV50=0.66, MOD50=13.31, logAge50=7.958
Cavallo et al. (2024) AV50=1.39, dMod50=13.24, logAge50=7.86, [Fe/H]50=-0.36
Hunt & Reffert (2024) MassJ=659.484, MassTot=592.117
Almeida et al. (2025) AV=1.044, Dist=3940, logAge=8.322, MassRk=438.6

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
FoF 1401 3.2 112.54 -14.02 0.24 -1.35 1.53 74.41 0.03