Collinder 458

(Harvard 21; MWSC 3774; OCL 273)

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C3
N_50
r_50
DC 17 6.4
Summary

Collinder 458 is a sparse, very loose object of very low C3 quality. It is located at a moderate distance from the Sun, near the mid-plane. It is poorly studied in the literature.

Warning: contains less than 25 stars with P>0.5 estimated.

Warning: the low UTI value and no obvious signs of duplication (C_dup=1.0) indicates that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
Dias et al. (2002) 358.525 61.767 4.48 -6.37
Kharchenko et al. (2012) 358.555 61.74 0.05 -3.47
Kharchenko et al. (2013) 358.555 61.74 0.05 -3.47
Kharchenko et al. (2016) 358.547 61.736
Bica et al. (2019) 358.571 61.735
Just et al. (2023) 358.547 61.736
           
UCC 358.623 61.78 0.255 -3.031 -1.092 -97.6
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

Collinder 458 UCC

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Fundamental parameters

Reference Values
Dias et al. (2002) E(B-V)=0.85, Dist=1937.0, Age=8.25
Kharchenko et al. (2012) E(B-V)=1.099, d=2501.0, logt=8.175
Kharchenko et al. (2013) E(B-V)=1.099, d=2501.0, logt=8.175
Kharchenko et al. (2016) E(B-V)=1.099, d=2501.0, logt=8.175
Just et al. (2023) logt=8.175, logmt=1.734

Search coordinates in Bayestar19

Cluster region map