Ruprecht 151

(OCL 606; MWSC 1309)

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C3
N_50
r_50
AB 39 7.6
Summary

Ruprecht 151 is a poorly populated, very dense object of high C3 quality. It is located at a relatively close distance from the Sun, above the mid-plane. It is very well-studied in the literature.

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
Piskunov et al. (2008) 115.316 -16.291
Kharchenko et al. (2012) 115.32 -16.29 -2.84 3.71
Loktin & Popova (2017) 115.32 -16.29 -4.716 2.892 33.5
Cantat-Gaudin et al. (2018) 115.315 -16.279 0.867 -4.272 3.242
Bica et al. (2019) 115.313 -16.247
Bossini et al. (2019) 115.315 -16.279
Cantat-Gaudin et al. (2020) 115.315 -16.279 0.867 -4.272 3.242
Dias et al. (2021) 115.303 -16.28 0.864 -4.286 3.262
Tarricq et al. (2022) 115.293 -16.294 0.912 -4.219 3.367
He et al. (2022) 115.295 -16.253 0.908 -4.259 3.368
Hunt & Reffert (2023) 115.3 -16.279 0.887 -4.238 3.334 21.567
Cavallo et al. (2024) 115.273 -16.299 0.89
Hunt & Reffert (2024) 115.3 -16.279 0.887 -4.238 3.334 21.567
Almeida et al. (2025) 115.303 -16.28
Hu & Soubiran (2025) 115.273 -16.299
           
UCC 115.293 -16.255 0.902 -4.239 3.369 22.807
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
Piskunov et al. (2008) E(B-V)=0.2, Dist=2100, logt=8.49, logMA=3.342
Kharchenko et al. (2012) e_bv=0.416, distance=1490, log_age=8.15, metallicity=-0.102
Loktin & Popova (2017) E(B-V)=0.082, Dist=3848, logt=8.81
Cantat-Gaudin et al. (2018) dmode=1115.6
Bossini et al. (2019) AV=0.587, Dist=10.359, logA=8.614, Fe/H=0.153
Cantat-Gaudin et al. (2020) AVNN=0.43, DistPc=1126.0, AgeNN=8.65
Dias et al. (2021) Av=0.542, Dist=1112, logage=8.793, [Fe/H]=0.048
Tarricq et al. (2022) Dist=1096, logAgeNN=8.69
He et al. (2022) A0=0.4, logAge=8.8
Hunt & Reffert (2023) AV50=0.259, diffAV50=0.49, MOD50=10.137, logAge50=8.676
Cavallo et al. (2024) AV50=0.3, dMod50=10.2, logAge50=8.92, [Fe/H]50=0.18
Hunt & Reffert (2024) MassJ=98.7300, MassTot=157.373
Almeida et al. (2025) AV=0.542, Dist=1112, logAge=8.793, MassRk=90.3
Hu & Soubiran (2025) MA22=-0.2, MA23f=-0.17, MZ23=-0.14, MK24=-0.14, MF24=-0.09

Search coordinates in Bayestar19

Cluster region map