Ruprecht 85

(VDBH83; FSR 1520; OCL 799; vdBergh-Hagen 83; ESO 167 15; MWSC 1746)

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C3
N_50
r_50
AA 373 2.3
Summary

Ruprecht 85 is a rich, very dense object of very high C3 quality. It is located at a large 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) 150.358 -55.117 -6.75 -0.84
Froebrich et al. (2007) 150.367 -55.117
Piskunov et al. (2008) 150.381 -55.013
Kharchenko et al. (2012) 150.42 -55.015 -4.8 4.45
Cantat-Gaudin et al. (2018) 150.36 -55.109 0.169 -4.443 3.241
Bica et al. (2019) 150.356 -55.115
Soubiran et al. (2018) 150.36 -55.109 22.93
Cantat-Gaudin et al. (2020) 150.36 -55.109 0.169 -4.443 3.241
Dias et al. (2021) 150.352 -55.111 0.172 -4.422 3.243 31.488
Hunt & Reffert (2023) 150.362 -55.109 0.182 -4.422 3.24 39.883
Cavallo et al. (2024) 150.347 -55.11 0.181
Hunt & Reffert (2024) 150.362 -55.109 0.182 -4.422 3.24 39.883
Almeida et al. (2025) 150.352 -55.111
           
UCC 150.36 -55.111 0.182 -4.419 3.241 23.451
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)=0.21, Dist=1400.0, Age=8.7
Piskunov et al. (2008) E(B-V)=0.21, Dist=1400, logt=8.7, logMA=2.047
Kharchenko et al. (2012) e_bv=0.167, distance=1286, log_age=8.7
Cantat-Gaudin et al. (2018) dmode=5041.8
Soubiran et al. (2018) dmode=5041.8
Cantat-Gaudin et al. (2020) AVNN=2.61, DistPc=4803.0, AgeNN=8.31
Dias et al. (2021) Av=3.081, Dist=4326, logage=8.348, [Fe/H]=0.01
Hunt & Reffert (2023) AV50=3.315, diffAV50=2.421, MOD50=13.424, logAge50=8.173
Cavallo et al. (2024) AV50=3.53, dMod50=13.26, logAge50=8.26, [Fe/H]50=-0.12
Hunt & Reffert (2024) MassJ=4852.63, MassTot=4880.59
Almeida et al. (2025) AV=3.081, Dist=4326, logAge=8.348, MassRk=1637.5

Search coordinates in Bayestar19

Cluster region map