Koposov 62

(MWSC 831)

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C3
N_50
r_50
AB 19 4.4
Summary

Koposov 62 is a sparse, very loose object of high C3 quality. It is located at a large distance from the Sun, above the mid-plane. It is moderately studied in the literature.

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

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

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
Dias et al. (2002) 94.508 24.711 1.86 -0.42
Koposov et al. (2008) 94.508 24.711
Glushkova et al. (2010) 94.508 24.711
Kharchenko et al. (2012) 94.509 24.695 -2.1 -4.84
Bica et al. (2019) 94.511 24.712
Donor et al. (2020) 94.509 24.695 -0.02 -0.43 51.8
           
UCC 94.533 24.755 0.172 0.242 -0.738
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

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Estimated members

Koposov 62 UCC

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Fundamental parameters

Reference Values
Dias et al. (2002) E(B-V)=0.34, Dist=2800.0, Age=9.4
Koposov et al. (2008) E(B-V)=0.34, Distance=2800, Age=9.4
Glushkova et al. (2010) E(B-V)=0.34, Dist=2800.0, Age=9.4
Kharchenko et al. (2012) e_bv=0.375, distance=3435, log_age=9.415
Donor et al. (2020) Fe/H=-0.27

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
HSC 1484 64.0 94.55 24.83 0.17 0.21 -0.72 0.09