Ruprecht 165

(OCL 881; ESO 172 01; MWSC 2036)

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C3
N_50
r_50
DC 18 7.0
Summary

Ruprecht 165 is a sparse, very loose object of very low C3 quality. It is located at a moderate distance from the Sun, above the mid-plane. It is poorly studied in the literature, with no articles listed in the last 6 years.

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) 187.146 -56.433 -14.37 -2.2
Kharchenko et al. (2012) 187.11 -56.43 -10.49 0.97
Bica et al. (2019) 187.136 -56.41
           
UCC 187.136 -56.407 0.29 -7.712 1.995
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

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Estimated members

Ruprecht 165 UCC

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Fundamental parameters

Reference Values
Dias et al. (2002) E(B-V)=0.645, Dist=2082.0, Age=9.115
Kharchenko et al. (2012) e_bv=0.645, distance=2082, log_age=9.115

Search coordinates in Bayestar19

Cluster region map