Ruprecht 64

(OCL 740; ESO 313 06; MWSC 1515)

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C3
N_50
r_50
CC 21 9.9
Summary

Ruprecht 64 is a sparse, very loose object of low C3 quality. It is located at a large distance from the Sun, above the mid-plane. It is moderately studied in the literature, with no articles listed in the last 6 years.

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) 129.333 -40.15 -5.17 5.84 26.9
Piskunov et al. (2007) 129.329 -40.145
Piskunov et al. (2008) 129.329 -40.145
Kharchenko et al. (2012) 129.27 -40.185 -6.15 5.95
Loktin & Popova (2017) 129.33 -40.149 -4.659 4.215 26.9
Bica et al. (2019) 129.493 -40.062
           
UCC 129.407 -40.188 0.134 -2.479 2.792 79.257
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

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Estimated members

Ruprecht 64 UCC

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Fundamental parameters

Reference Values
Dias et al. (2002) E(B-V)=0.06, Dist=800.0, Age=8.45
Piskunov et al. (2007) E(B-V)=0.06, Dist=800, logt=8.45, logM=2.859
Piskunov et al. (2008) E(B-V)=0.06, Dist=800, logt=8.45, logM=3.33, logMA=3.32
Kharchenko et al. (2012) e_bv=0.125, distance=619, log_age=8.45
Loktin & Popova (2017) E(B-V)=0.598, Dist=791, logt=7.851

Search coordinates in Bayestar19

Cluster region map