DBSB 72

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.0 0.1 0.38 0.0 1.0
C3
N_50
r_50
CB 15 3.1
Summary

DBSB 72 is a sparse, very loose object of low C3 quality. It is located at a large distance from the Sun, below the mid-plane. It is rarely studied in the literature.

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

Warning: the low UTI value and no obvious signs of duplication (C_dup=1.0) indicates that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
Kharchenko et al. (2012) 176.487 -65.555 – -6.28 3.72 –
He et al. (2023) 176.484 -65.551 0.272 -5.783 1.107 –
           
UCC 176.511 -65.553 0.161 -5.957 0.901 -13.588
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

DBSB 72 UCC

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Fundamental parameters

Reference Values
Kharchenko et al. (2012) e_bv=2.29, distance=4494, log_age=6.1
He et al. (2023) A0=3.1, m-M=13.3, logA=6.3

Search coordinates in Bayestar19

Cluster region map