CWNU 1634

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.0 0.36 0.75 0.0 1.0
C3
N_50
r_50
AB 22 6.3
Summary

CWNU 1634 is a sparse, loose object of high C3 quality. It is located at a relatively close distance from the Sun, below the mid-plane. It was recently reported in the literature.

This object shares a large 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
He et al. (2023) 296.441 14.812 0.529 -1.474 -4.882 6.02
           
UCC 296.431 14.822 0.525 -1.456 -4.882 6.023
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 1634 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2023) A0=0.8, m-M=11.2, logAge=8.4

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
Theia 3886 88.0 296.42 14.81 0.52 -1.46 -4.86 – 0.03