Ruprecht 115

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C3
N_50
r_50
AA 130 2.2
Summary

Ruprecht 115 is a rich, very dense object of very high C3 quality. It is located at a moderate distance from the Sun, near the mid-plane. It is well-studied in the literature.

This object shares a small percentage of members with a later reported entry.

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
Dias et al. (2002) 243.217 -52.4 -2.49 -4.8
Kharchenko et al. (2012) 243.24 -52.427 -3.73 -6.26
Cantat-Gaudin et al. (2018) 243.215 -52.393 0.366 -4.333 -4.546
Soubiran et al. (2018) 243.215 -52.393 -40.5
Bossini et al. (2019) 243.215 -52.393
Cantat-Gaudin et al. (2020) 243.215 -52.393 0.366 -4.333 -4.546
Rain et al. (2021) 243.215 -52.393 0.366 -4.333 -4.546
Jaehnig et al. (2021) 243.214 -52.392 0.382 -4.371 -4.569
Hunt & Reffert (2023) 243.214 -52.397 0.39 -4.313 -4.587 -39.897
Cavallo et al. (2024) 243.217 -52.397 0.39
Hunt & Reffert (2024) 243.214 -52.397 0.39 -4.313 -4.587 -39.897
           
UCC 243.213 -52.396 0.378 -4.353 -4.556 -41.183
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

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Estimated members

Explore data in Colab

Fundamental parameters

Reference Values
Dias et al. (2002) E(B-V)=0.65, Dist=2160.0, Age=8.78, [Fe/H]=0.04
Kharchenko et al. (2012) e_bv=0.937, distance=1948, log_age=9.135
Cantat-Gaudin et al. (2018) dmode=2529.9
Soubiran et al. (2018) dmode=2529.9
Bossini et al. (2019) AV=2.317, Dist=11.908, logA=8.474, Fe/H=-0.102
Cantat-Gaudin et al. (2020) AVNN=2.25, DistPc=2355.0, AgeNN=8.37
Rain et al. (2021) E(B-V)=0.65, Dist=2529.9, log(Age)=8.78, NBSS=0
Jaehnig et al. (2021) dmode=2.586
Hunt & Reffert (2023) AV50=2.963, diffAV50=1.826, MOD50=11.859, logAge50=8.196
Cavallo et al. (2024) AV50=3.56, dMod50=11.27, logAge50=8.05, [Fe/H]50=-0.6
Hunt & Reffert (2024) MassJ=953.975, MassTot=953.975

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
OC 0646 21.5 243.21 -52.39 0.4 -4.36 -4.53 -39.97 0.0