Cmg 903

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C3
N_50
r_50
DC 17 6.7
Summary

Cmg 903 is a sparse, very loose object of very low C3 quality. It is located at a large distance from the Sun, well below the mid-plane. It is rarely studied in the literature, with no articles listed in the last 6 years.

This object shares a moderate percentage of members with at least one entry reported in the same catalogue.

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
Bica et al. (2019) 64.001 32.312
           
UCC 63.981 32.292 0.158 -0.102 -0.958 -19.146
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

Cmg 903 UCC

Explore data in Colab

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
Cmg 902 40.0 63.78 32.25 0.21 -0.05 -0.46 -17.91 0.29
HSC 1293 4.0 63.79 32.27 0.19 0.26 -0.66 -12.1 0.04