DBSB 175

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C3
N_50
r_50
DC 16 7.3
Summary

DBSB 175 is a sparse, very loose object of very low C3 quality. It is located at a moderate distance from the Sun, near the mid-plane. It is rarely studied in the literature, with no articles listed in the last 13 years.

This object shares a small percentage of members with 2 later reported entries.

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) 253.148 -43.396 -2.69 -2.03
           
UCC 253.065 -43.421 0.414 -1.262 -3.815 -23.938
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

DBSB 175 UCC

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Fundamental parameters

Reference Values
Kharchenko et al. (2012) e_bv=1.249, distance=3798, log_age=6.0

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
Bica 513 20.0 253.42 -43.52 0.44 -1.4 -3.84 -16.7 0.08
Ryu 82 4.0 253.17 -43.2 0.44 -1.39 -3.38 -17.67 0.22