Ruprecht 31

(OCL 711; ESO 368 09; MWSC 1317)

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C3
N_50
r_50
BA 26 39.7
Summary

Ruprecht 31 is a poorly populated, very loose object of high C3 quality. It is located at a very close distance from the Sun, near the mid-plane. It is moderately studied in the literature.

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

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
Piskunov et al. (2008) 115.737 -35.602
Kharchenko et al. (2012) 115.748 -35.593 -4.9 3.65
Loktin & Popova (2017) 115.74 -35.597 -11.57 7.746
Angelo et al. (2019) 115.75 -35.6
Bica et al. (2019) 115.741 -35.588
He et al. (2022) 115.367 -35.111 2.313 -8.168 4.314
           
UCC 115.71 -35.304 2.3 -8.254 4.267 17.399
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

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Estimated members

Ruprecht 31 UCC

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Fundamental parameters

Reference Values
Piskunov et al. (2008) E(B-V)=0.09, Dist=480, logt=8.56, logMA=0.888
Kharchenko et al. (2012) e_bv=0.104, distance=541, log_age=8.65
Loktin & Popova (2017) E(B-V)=0.391, Dist=2716, logt=8.66
Angelo et al. (2019) dsun=2.29, Age=0.79, Mphot=27
He et al. (2022) A0=0.6, logAge=7.55

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
OCSN 84 92.3 115.03 -34.48 2.3 -8.25 4.28 16.39 0.22