CWNU 1835

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.0 0.2 0.38 0.0 1.0
C3
N_50
r_50
CB 21 4.4
Summary

CWNU 1835 is a sparse, very loose object of low C3 quality. It is located at a moderate 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) 96.604 8.267 0.29 0.178 -1.754 –
           
UCC 96.583 8.231 0.278 0.179 -1.761 46.5
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 1835 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2023) A0=1.55, m-M=12.75, logAge=8.7

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
Theia 2615 84.0 96.6 8.22 0.27 0.17 -1.78 46.5 0.04