CWNU 3776

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.0 1.0 0.38 0.0 0.08
C3
N_50
r_50
CB 23 4.1
Summary

CWNU 3776 is a sparse, very dense 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.

Warning: This is very 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) 99.98 6.032 0.648 -1.528 0.969 –
           
UCC 99.975 6.047 0.66 -1.53 0.969 –
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 3776 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2023) A0=1.7, m-M=10.85, logA=7.5

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
Desvoivres 2 92.0 99.97 6.06 0.65 -1.53 0.96 – 0.41