CMa05

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.0 0.24 0.12 0.0 1.0
C3
N_50
r_50
DC 24 11.8
Summary

CMa05 is a sparse, very loose object of very low C3 quality. It is located at a relatively close distance from the Sun, near the mid-plane. It is rarely studied in the literature.

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

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
Santos-Silva et al. (2021) 105.32 -11.2 0.78 -2.98 0.79 –
           
UCC 105.264 -11.289 0.766 -3.058 0.862 19.535
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CMa05 UCC

Explore data in Colab

Fundamental parameters

Reference Values
Santos-Silva et al. (2021) AVPM=1.27, AVPf=1.11, DPM=1229, DPf=1130.0, AgeM=17.0, AgeF=18, [Fe/H]M=-0.14, [Fe/H]f=-0.1

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 76 24.0 104.97 -11.16 0.88 -2.9 0.68 31.15 0.18