Ruprecht 47

(OCL 699; ESO 430 08; FSR 1344; MWSC 1419)

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C3
N_50
r_50
AB 121 3.0
Summary

Ruprecht 47 is a rich, 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
Dias et al. (2002) 120.579 -31.067 -1.68 -0.45 59.7
Piskunov et al. (2008) 120.576 -31.066
Kharchenko et al. (2012) 120.585 -31.07 0.14 0.56
Cantat-Gaudin et al. (2018) 120.57 -31.074 0.234 -2.5 2.727
Bica et al. (2019) 120.576 -31.066
Soubiran et al. (2018) 120.57 -31.074 74.2
Cantat-Gaudin et al. (2020) 120.57 -31.074 0.234 -2.5 2.727
Dias et al. (2021) 120.565 -31.071 0.241 -2.507 2.73
Hunt & Reffert (2023) 120.57 -31.073 0.26 -2.44 2.723 89.241
Cavallo et al. (2024) 120.564 -31.083 0.261
Celli et al. (2024) 120.57 -31.074
Hunt & Reffert (2024) 120.57 -31.073 0.26 -2.44 2.723 89.241
Almeida et al. (2025) 120.565 -31.071
           
UCC 120.568 -31.075 0.256 -2.446 2.727 92.011
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)=0.28, Dist=3006.0, Age=7.89
Piskunov et al. (2008) E(B-V)=0.25, Dist=3006, logt=8.07, logMA=3.303
Kharchenko et al. (2012) e_bv=0.291, distance=2892, log_age=8.18
Cantat-Gaudin et al. (2018) dmode=3799.2
Soubiran et al. (2018) dmode=3799.2
Cantat-Gaudin et al. (2020) AVNN=0.93, DistPc=3720.0, AgeNN=7.47
Dias et al. (2021) Av=1.086, Dist=3431, logage=8.144, [Fe/H]=-0.123
Hunt & Reffert (2023) AV50=0.439, diffAV50=0.377, MOD50=12.775, logAge50=8.39
Cavallo et al. (2024) AV50=0.84, dMod50=12.87, logAge50=8.32, [Fe/H]50=0.48
Celli et al. (2024) Age=29.5, Mc=334.6
Hunt & Reffert (2024) MassJ=564.005, MassTot=598.275
Almeida et al. (2025) AV=1.086, Dist=3431, logAge=8.144, MassRk=386.2

Search coordinates in Bayestar19

Cluster region map