Ruprecht 105

(OCL 886; ESO 131 12; Slotegraaf 41; MWSC 2047; FoF 2153)

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C3
N_50
r_50
AA 62 5.1
Summary

Ruprecht 105 is a moderately populated, very dense object of very high C3 quality. It is located at a moderate distance from the Sun, above the mid-plane. It is very well-studied in the literature.

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Positions

Reference RA DEC Plx pmRA pmDE Rv
Dias et al. (2002) 188.558 -61.567 -1.53 -0.68
Piskunov et al. (2008) 188.548 -61.563
Kharchenko et al. (2012) 188.475 -61.575 -8.5 -0.64
Cantat-Gaudin et al. (2018) 188.694 -61.592 0.46 -5.986 -0.001
Bica et al. (2019) 188.61 -61.575
Soubiran et al. (2018) 188.694 -61.592 -4.38
Liu & Pang (2019) 188.696 -61.58 0.466 -5.914 -0.066
Cantat-Gaudin et al. (2020) 188.694 -61.592 0.46 -5.986 -0.001
Dias et al. (2021) 188.721 -61.606 0.459 -5.993 -0.006 -3.941
Hunt & Reffert (2023) 188.637 -61.595 0.465 -6.017 0.025 -2.742
Cavallo et al. (2024) 188.712 -61.58 0.469
Hunt & Reffert (2024) 188.637 -61.595 0.465 -6.017 0.025 -2.742
Almeida et al. (2025) 188.721 -61.606
           
UCC 188.704 -61.588 0.472 -6.007 0.0 -2.63
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)=0.05, Dist=950.0, Age=9.01
Piskunov et al. (2008) E(B-V)=0.05, Dist=950, logt=9.01, logMA=1.889
Kharchenko et al. (2012) e_bv=0.05, distance=1250, log_age=9.1
Cantat-Gaudin et al. (2018) dmode=2046.7
Soubiran et al. (2018) dmode=2046.7
Liu & Pang (2019) Age=0.955, Z=-0.25
Cantat-Gaudin et al. (2020) AVNN=1.5, DistPc=2050.0, AgeNN=8.59
Dias et al. (2021) Av=1.867, Dist=1905, logage=8.208, [Fe/H]=0.2
Hunt & Reffert (2023) AV50=1.658, diffAV50=1.311, MOD50=11.464, logAge50=8.404
Cavallo et al. (2024) AV50=1.81, dMod50=11.4, logAge50=8.53, [Fe/H]50=0.15
Hunt & Reffert (2024) MassJ=476.423, MassTot=501.716
Almeida et al. (2025) AV=1.867, Dist=1905, logAge=8.208, MassRk=178.5

Search coordinates in Bayestar19

Cluster region map