Ruprecht 60

(VDBH 31; OCL 751; vdBergh-Hagen 31; ESO 259 07; FSR 1420; MWSC 1485)

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C3
N_50
r_50
AA 286 2.4
Summary

Ruprecht 60 is a rich, very dense object of very high C3 quality. It is located at a moderate distance from the Sun, below the mid-plane. It is very well-studied in the literature.

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
Dias et al. (2002) 126.108 -47.214 -1.29 3.5
Glushkova et al. (2010) 126.096 -47.21
Kharchenko et al. (2012) 126.108 -47.2 -4.6 5.39
Cantat-Gaudin et al. (2018) 126.105 -47.207 0.186 -3.788 5.401
Bica et al. (2019) 126.118 -47.206
Soubiran et al. (2018) 126.105 -47.207 53.24
Cantat-Gaudin et al. (2020) 126.105 -47.207 0.186 -3.788 5.401
Dias et al. (2021) 126.101 -47.199 0.186 -3.779 5.387
Hunt & Reffert (2023) 126.11 -47.211 0.218 -3.744 5.436 53.362
Cavallo et al. (2024) 126.106 -47.205 0.214
Hunt & Reffert (2024) 126.11 -47.211 0.218 -3.744 5.436 53.362
Almeida et al. (2025) 126.101 -47.199
Hu & Soubiran (2025) 126.106 -47.205
           
UCC 126.105 -47.21 0.216 -3.745 5.434 52.642
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

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Estimated members

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Fundamental parameters

Reference Values
Dias et al. (2002) E(B-V)=0.64, Dist=6160.0, Age=8.6
Glushkova et al. (2010) E(B-V)=0.57, Dist=3700.0, Age=8.65
Kharchenko et al. (2012) e_bv=0.639, distance=5739, log_age=8.6
Cantat-Gaudin et al. (2018) dmode=4648.4
Soubiran et al. (2018) dmode=4648.4
Cantat-Gaudin et al. (2020) AVNN=1.05, DistPc=4322.0, AgeNN=8.99
Dias et al. (2021) Av=1.558, Dist=3959, logage=8.929, [Fe/H]=-0.125
Hunt & Reffert (2023) AV50=1.286, diffAV50=1.306, MOD50=13.061, logAge50=8.836
Cavallo et al. (2024) AV50=1.52, dMod50=12.53, logAge50=9.08, [Fe/H]50=-0.45
Hunt & Reffert (2024) MassJ=1695.43, MassTot=1729.71
Almeida et al. (2025) AV=1.558, Dist=3959, logAge=8.929, MassRk=738.4
Hu & Soubiran (2025) MA22=-0.21, MA23f=-0.38, MA23g=-0.29, MZ23=-0.64, MK24=-0.32, MF24=-0.32

Search coordinates in Bayestar19

Cluster region map