Ruprecht 36

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C3
N_50
r_50
AB 126 3.7
Summary

Ruprecht 36 is a rich, very dense object of high C3 quality. It is located at a moderate 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) 117.096 -26.3 -3.67 2.29
Kharchenko et al. (2012) 117.097 -26.29 -5.15 3.04
Loktin & Popova (2017) 117.09 -26.299 -4.843 1.422
Cantat-Gaudin et al. (2018) 117.096 -26.287 0.34 -2.768 0.903
Soubiran et al. (2018) 117.096 -26.287 41.9
Cantat-Gaudin et al. (2020) 117.096 -26.287 0.34 -2.768 0.903
Dias et al. (2021) 117.095 -26.281 0.348 -2.779 0.9
Rain et al. (2021) 117.096 -26.287 0.34 -2.768 0.903
Jaehnig et al. (2021) 117.099 -26.29 0.372 -2.725 0.902
Hunt & Reffert (2023) 117.09 -26.29 0.354 -2.691 0.931 68.601
Cavallo et al. (2024) 117.096 -26.278 0.361
Hunt & Reffert (2024) 117.09 -26.29 0.354 -2.691 0.931 68.601
Almeida et al. (2025) 117.095 -26.281
           
UCC 117.093 -26.291 0.363 -2.694 0.93
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)=0.166, Dist=1681.0, Age=7.606
Kharchenko et al. (2012) e_bv=0.15, distance=1821, log_age=8.28
Loktin & Popova (2017) E(B-V)=0.166, Dist=1707, logt=7.643
Cantat-Gaudin et al. (2018) dmode=2709.2
Soubiran et al. (2018) dmode=2709.2
Cantat-Gaudin et al. (2020) AVNN=0.63, DistPc=2706.0, AgeNN=7.75
Dias et al. (2021) Av=0.859, Dist=2485, logage=8.015, [Fe/H]=-0.13
Rain et al. (2021) E(B-V)=0.16, Dist=2709.2, log(Age)=7.6, NBSS=0
Jaehnig et al. (2021) dmode=2.765
Hunt & Reffert (2023) AV50=0.321, diffAV50=0.984, MOD50=11.946, logAge50=8.284
Cavallo et al. (2024) AV50=0.74, dMod50=11.69, logAge50=8.44, [Fe/H]50=-0.37
Hunt & Reffert (2024) MassJ=293.547, MassTot=298.244
Almeida et al. (2025) AV=0.859, Dist=2485, logAge=8.015, MassRk=370.1

Search coordinates in Bayestar19

Cluster region map