Kronberger 39

(DSH J1054.2-6144; MWSC 1868)

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C3
N_50
r_50
DC 22 5.8
Summary

Kronberger 39 is a sparse, very loose object of very low C3 quality. It is located at a large distance from the Sun, below the mid-plane. It is poorly studied in the literature.

Warning: contains less than 25 stars with P>0.5 estimated.

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Positions

Reference RA DEC Plx pmRA pmDE Rv
Dias et al. (2002) 163.558 -61.738 -3.91 6.07
Kronberger et al. (2006) 163.557 -61.738
Kharchenko et al. (2012) 163.559 -61.733 -3.91 6.07
Bica et al. (2019) 163.545 -61.74
Perren et al. (2022) 163.557 -61.738
           
UCC 163.575 -61.747 0.116 -4.731 1.922 46.722
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

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Estimated members

Kronberger 39 UCC

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Fundamental parameters

Reference Values
Dias et al. (2002) E(B-V)=0.9, Dist=11100.0
Kronberger et al. (2006) E(B-V)=0.9, Dist=11.1
Kharchenko et al. (2012) e_bv=0.999, distance=4372, log_age=6.0
Perren et al. (2022) E(B-V)=0.78, dm=15.57, logt=9.45, FeH=-0.11, Mass=13000, bfr=0.75

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Cluster region map