Ruprecht 176

(MWSC 2373)

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C3
N_50
r_50
AA 381 4.9
Summary

Ruprecht 176 is a rich, very dense object of very high C3 quality. It is located at a moderate distance from the Sun, near the mid-plane. It is well-studied in the literature.

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
Dias et al. (2002) 243.7 -51.333 -2.99 -2.9
Kharchenko et al. (2013) 243.66 -51.333 -4.3 -3.01
Kharchenko et al. (2016) 243.649 -51.332
Cantat-Gaudin et al. (2018) 243.676 -51.332 0.335 -2.644 -2.984
Soubiran et al. (2018) 243.676 -51.332 -52.19
Bossini et al. (2019) 243.676 -51.332
Cantat-Gaudin et al. (2020) 243.676 -51.332 0.335 -2.644 -2.984
Dias et al. (2021) 243.681 -51.333 0.338 -2.677 -2.99 -52.246
Just et al. (2023) 243.649 -51.332
Hunt & Reffert (2023) 243.671 -51.333 0.365 -2.703 -2.991 -52.27
Cavallo et al. (2024) 243.679 -51.339 0.363
Hunt & Reffert (2024) 243.671 -51.333 0.365 -2.703 -2.991 -52.27
Almeida et al. (2025) 243.681 -51.333
           
UCC 243.675 -51.333 0.357 -2.684 -2.992 -52.249
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)=0.479, Dist=2686.0, Age=8.76
Kharchenko et al. (2013) E(B-V)=0.479, d=2686.0, logt=8.76
Kharchenko et al. (2016) E(B-V)=0.479, d=2686.0, logt=8.76
Cantat-Gaudin et al. (2018) dmode=2749.3
Soubiran et al. (2018) dmode=2749.3
Bossini et al. (2019) AV=1.678, Dist=12.059, logA=8.168, Fe/H=0.0
Cantat-Gaudin et al. (2020) AVNN=1.66, DistPc=2615.0, AgeNN=8.08
Dias et al. (2021) Av=1.865, Dist=2220, logage=8.115, [Fe/H]=0.179
Just et al. (2023) logt=8.76, logmt=2.786
Hunt & Reffert (2023) AV50=1.751, diffAV50=1.467, MOD50=11.943, logAge50=8.332
Cavallo et al. (2024) AV50=2.38, dMod50=11.16, logAge50=8.21, [Fe/H]50=-0.9
Hunt & Reffert (2024) MassJ=1616.46, MassTot=1692.83
Almeida et al. (2025) AV=1.865, Dist=2220, logAge=8.115, MassRk=738.8

Search coordinates in Bayestar19

Cluster region map