CWNU 202

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.26 0.11 0.75 0.0 1.0
C3
N_50
r_50
AB 26 14.6
Summary

CWNU 202 is a poorly populated, very loose object of high 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 significant percentage of members with a later reported entry.

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) 303.537 34.572 0.62 -0.83 -3.64 –
           
UCC 303.485 34.564 0.624 -0.839 -3.641 -24.642
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

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Estimated members

CWNU 202 UCC

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Fundamental parameters

Reference Values
He et al. (2022) AG=1.4, m-M=10.6, logAge=7.8, Z=0.008

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
Theia 2007 65.4 303.43 34.46 0.62 -0.88 -3.64 -36.82 0.07