Ruprecht 13

(OCL 631; ESO 491 17; MWSC 1116)

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C3
N_50
r_50
DC 7 8.5
Summary

Ruprecht 13 is a sparse, very loose object of very low C3 quality. It is located at a large distance from the Sun, well below 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.

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
Dias et al. (2002) 106.963 -25.87 -2.15 -0.96
Kharchenko et al. (2012) 107.002 -25.88 -5.09 5.58
Loktin & Popova (2017) 106.98 -25.88 -4.093 4.732
Bica et al. (2019) 107.012 -25.86
           
UCC 106.94 -25.827 0.114 -0.912 1.453
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

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Estimated members

Ruprecht 13 UCC

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Fundamental parameters

Reference Values
Dias et al. (2002) E(B-V)=0.26, Dist=1300.0, Age=9.0
Kharchenko et al. (2012) e_bv=0.354, distance=2276, log_age=8.89
Loktin & Popova (2017) E(B-V)=0.223, Dist=2969, logt=8.88

Search coordinates in Bayestar19

Cluster region map