Ruprecht 53

(OCL 682; ESO 494 32; MWSC 1442)

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C3
N_50
r_50
AB 57 11.9
Summary

Ruprecht 53 is a moderately populated, dense object of high C3 quality. It is located at a relatively close distance from the Sun, above 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
Dias et al. (2002) 122.725 -26.0 -2.0 4.52
Piskunov et al. (2008) 122.692 -26.993
Kharchenko et al. (2012) 122.68 -26.94 -0.34 5.63
Bica et al. (2019) 122.717 -26.991
Hunt & Reffert (2023) 122.741 -27.003 0.956 -2.877 0.99 11.802
Cavallo et al. (2024) 122.728 -27.037 0.957
Hunt & Reffert (2024) 122.741 -27.003 0.956 -2.877 0.99 11.802
           
UCC 122.737 -27.027 0.968 -2.864 1.004 11.48
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)=0.11, Dist=1700.0, Age=8.59
Piskunov et al. (2008) E(B-V)=0.11, Dist=1700, logt=8.59, logMA=2.721
Kharchenko et al. (2012) e_bv=0.271, distance=1523, log_age=8.86
Hunt & Reffert (2023) AV50=0.09, diffAV50=0.54, MOD50=9.929, logAge50=8.535
Cavallo et al. (2024) AV50=0.19, dMod50=10.0, logAge50=8.49, [Fe/H]50=-0.07
Hunt & Reffert (2024) MassJ=125.514, MassTot=146.983

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 1026 77.2 122.75 -27.04 0.97 -2.86 1.02 11.15 0.0