CWNU 484

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C3
N_50
r_50
CB 15 11.9
Summary

CWNU 484 is a sparse, very loose object of low C3 quality. It is located at a relatively close distance from the Sun, near the mid-plane. It was recently reported in the literature.

This object shares a small 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
He et al. (2022) 275.374 -17.484 0.58 0.36 -1.8
           
UCC 275.277 -17.481 0.552 0.378 -1.819
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 484 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2022) AG=2.4, m-M=12.15, logAge=7.1, Z=0.04

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 303 16.0 275.42 -17.53 0.52 0.52 -1.82 30.78 0.13