CWNU 3772

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.0 0.75 0.38 0.0 0.16
C3
N_50
r_50
CB 23 2.0
Summary

CWNU 3772 is a sparse, dense object of low C3 quality. It is located at a moderate distance from the Sun, near the mid-plane. It was recently reported in the literature.

Warning: This is likely a duplicate object, which shares a large percentage of members with at least one previously reported entry.

Warning: contains less than 25 stars with P>0.5 estimated.

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
He et al. (2023) 7.501 62.836 0.226 -2.037 -0.444 –
           
UCC 7.501 62.843 0.235 -2.031 -0.423 -72.101
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 3772 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2023) A0=2.9, m-M=12.95, logA=7.2

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
Theia 1851 84.0 7.51 62.84 0.23 -2.03 -0.42 -72.1 0.35