Collinder 304

(NGC 6152; MWSC 2423; OCL 961; ESO 179 09)

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C3
N_50
r_50
AA 267 6.9
Summary

Collinder 304 is a rich, very dense object of very high C3 quality. It is located at a relatively close distance from the Sun, below the mid-plane. It is very well-studied in the literature.

This object shares a 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) 248.188 -52.643 -1.85 -4.87
Kharchenko et al. (2003) 248.17 -52.62 -1.85 -3.18
Kharchenko et al. (2005) 248.17 -52.64 -2.06 -2.5
Piskunov et al. (2007) 248.158 -52.638
Piskunov et al. (2008) 248.158 -52.638
Kharchenko et al. (2013) 248.175 -52.64 -2.0 -4.35
Kharchenko et al. (2016) 248.163 -52.639
Cantat-Gaudin et al. (2018) 248.213 -52.629 0.594 -2.511 -4.98
Bica et al. (2019) 248.17 -52.645
Soubiran et al. (2018) 248.213 -52.629 -35.7
Bossini et al. (2019) 248.213 -52.629
Monteiro & Dias (2019) 248.213 -52.629 -2.536 -4.987 2.204
Cantat-Gaudin et al. (2020) 248.213 -52.629 0.594 -2.511 -4.98
Dias et al. (2021) 248.216 -52.624 0.594 -2.519 -4.972 -35.513
Rain et al. (2021) 248.213 -52.629 0.594 -2.511 -4.98
Just et al. (2023) 248.163 -52.639
Cordoni et al. (2023) 248.216 -52.624 0.594 -2.519 -4.972
Hunt & Reffert (2023) 248.158 -52.621 0.608 -2.581 -4.993 -34.365
Cavallo et al. (2024) 248.222 -52.631 0.608
Hunt & Reffert (2024) 248.158 -52.621 0.608 -2.581 -4.993 -34.365
Almeida et al. (2025) 248.216 -52.624
           
UCC 248.212 -52.637 0.609 -2.565 -4.99 -35.927
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

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Estimated members

Explore data in Colab

Fundamental parameters

Reference Values
Dias et al. (2002) E(B-V)=0.3, Dist=1030.0
Kharchenko et al. (2003) E(B-V)=0.3, Dist=1030
Kharchenko et al. (2005) E(B-V)=0.2, Dist=1030, logt=8.65
Piskunov et al. (2007) E(B-V)=0.2, Dist=1030, logt=8.65, logM=2.565
Piskunov et al. (2008) E(B-V)=0.2, Dist=1030, logt=8.65, logM=3.097, logMA=3.049
Kharchenko et al. (2013) E(B-V)=0.198, d=1031.0, logt=8.63
Kharchenko et al. (2016) E(B-V)=0.198, d=1031.0, logt=8.63
Cantat-Gaudin et al. (2018) dmode=1606.1
Soubiran et al. (2018) dmode=1606.1
Bossini et al. (2019) AV=1.059, Dist=10.986, logA=8.236, Fe/H=0.0
Monteiro & Dias (2019) E(B-V)=0.383, Dist=1.536, logAge=8.433, Z=0.022
Cantat-Gaudin et al. (2020) AVNN=1.01, DistPc=1618.0, AgeNN=8.35
Dias et al. (2021) Av=1.128, Dist=1422, logage=8.386, [Fe/H]=0.131
Rain et al. (2021) E(B-V)=0.2, Dist=1606.1, log(Age)=8.65, NBSS=0
Just et al. (2023) logt=8.63, logmt=1.932
Cordoni et al. (2023) Av=1.128, Dist=10.764, logAge=8.386, [Fe/H]=0.131, mass-single=3525.27, fbin-tot=0.556, fbss-MS=0.0
Hunt & Reffert (2023) AV50=1.013, diffAV50=0.85, MOD50=10.941, logAge50=8.189
Cavallo et al. (2024) AV50=1.13, dMod50=10.76, logAge50=8.46, [Fe/H]50=0.14
Hunt & Reffert (2024) MassJ=1427.35, MassTot=1437.79
Almeida et al. (2025) AV=1.128, Dist=1422, logAge=8.386, MassRk=486.3

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
OC 0654 13.1 248.25 -52.58 0.62 -2.56 -5.03 -35.18 0.0