Ruprecht 34

(Berkeley 38; OCL 628; ESO 560 10; MWSC 1330)

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C3
N_50
r_50
BB 100 2.3
Summary

Ruprecht 34 is a rich, very dense object of intermediate C3 quality. It is located at a moderate 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
Dias et al. (2002) 116.483 -20.39 -3.01 0.82
Piskunov et al. (2008) 116.471 -20.383
Kharchenko et al. (2012) 116.487 -20.385 -4.87 0.6
Cantat-Gaudin et al. (2018) 116.478 -20.386 0.357 -2.129 1.044
Bica et al. (2019) 116.46 -20.365
Soubiran et al. (2018) 116.478 -20.386 46.44
Bossini et al. (2019) 116.478 -20.386
Cantat-Gaudin et al. (2020) 116.478 -20.386 0.357 -2.129 1.044
Dias et al. (2021) 116.472 -20.388 0.391 -2.145 1.05 46.496
Hunt & Reffert (2023) 116.482 -20.385 0.35 -2.176 1.042 46.375
Cavallo et al. (2024) 116.479 -20.388 0.351
Hunt & Reffert (2024) 116.482 -20.385 0.35 -2.176 1.042 46.375
Almeida et al. (2025) 116.472 -20.388
           
UCC 116.483 -20.386 0.351 -2.15 1.031 46.392
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)=0.0, Dist=2630.0, Age=9.0
Piskunov et al. (2008) E(B-V)=0.1, Dist=800, logt=8.9, logMA=1.529
Kharchenko et al. (2012) e_bv=0.146, distance=893, log_age=9.1
Cantat-Gaudin et al. (2018) dmode=2593.7
Soubiran et al. (2018) dmode=2593.7
Bossini et al. (2019) AV=0.362, Dist=11.82, logA=8.865, Fe/H=0.0
Cantat-Gaudin et al. (2020) AVNN=0.49, DistPc=2525.0, AgeNN=8.66
Dias et al. (2021) Av=0.977, Dist=2518, logage=8.611, [Fe/H]=-0.1
Hunt & Reffert (2023) AV50=0.8, diffAV50=0.885, MOD50=12.006, logAge50=8.597
Cavallo et al. (2024) AV50=0.8, dMod50=11.98, logAge50=8.51, [Fe/H]50=0.13
Hunt & Reffert (2024) MassJ=339.894, MassTot=409.145
Almeida et al. (2025) AV=0.977, Dist=2518, logAge=8.611, MassRk=306.1

Search coordinates in Bayestar19

Cluster region map