Ruprecht 50

(VDBH 17; OCL 698; vdBergh-Hagen 17; ESO 430 12; MWSC 1424; FoF 960)

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C3
N_50
r_50
AB 82 3.3
Summary

Ruprecht 50 is a moderately populated, very dense object of high C3 quality. It is located at a moderate distance from the Sun, near the mid-plane. It is very well-studied in the literature.

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
Kharchenko et al. (2012) 120.877 -30.86 0.42 -1.15
Cantat-Gaudin et al. (2018) 120.872 -30.873 0.414 -1.726 2.352
Bica et al. (2019) 120.851 -30.859
Soubiran et al. (2018) 120.872 -30.873 51.08
Bossini et al. (2019) 120.872 -30.873
Liu & Pang (2019) 120.873 -30.881 0.388 -1.913 2.446
Cantat-Gaudin et al. (2020) 120.872 -30.873 0.414 -1.726 2.352
Dias et al. (2021) 120.869 -30.876 0.413 -1.723 2.363
Perren et al. (2022) 120.872 -30.873
Hunt & Reffert (2023) 120.876 -30.868 0.417 -1.771 2.371 48.949
Cavallo et al. (2024) 120.86 -30.868 0.423
Hunt & Reffert (2024) 120.876 -30.868 0.417 -1.771 2.371 48.949
Almeida et al. (2025) 120.869 -30.876
           
UCC 120.866 -30.874 0.425 -1.77 2.37 48.954
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
Kharchenko et al. (2012) e_bv=0.104, distance=1834, log_age=8.775
Cantat-Gaudin et al. (2018) dmode=2259.8
Soubiran et al. (2018) dmode=2259.8
Bossini et al. (2019) AV=0.575, Dist=11.709, logA=8.578, Fe/H=0.0
Liu & Pang (2019) Age=0.576, Z=-0.25
Cantat-Gaudin et al. (2020) AVNN=0.61, DistPc=2157.0, AgeNN=8.66
Dias et al. (2021) Av=0.76, Dist=2064, logage=8.715, [Fe/H]=-0.034
Perren et al. (2022) E(B-V)=0.52, dm=16.31, logt=9.7, FeH=0.15, Mass=170000, bfr=0.48
Hunt & Reffert (2023) AV50=0.422, diffAV50=0.728, MOD50=11.642, logAge50=8.659
Cavallo et al. (2024) AV50=0.89, dMod50=11.7, logAge50=8.68, [Fe/H]50=-0.15
Hunt & Reffert (2024) MassJ=386.142, MassTot=397.585
Almeida et al. (2025) AV=0.76, Dist=2064, logAge=8.715, MassRk=221.5

Search coordinates in Bayestar19

Cluster region map