CWNU 3777

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.26 1.0 1.0 0.0 0.12
C3
N_50
r_50
AA 26 0.7
Summary

CWNU 3777 is a poorly populated, very dense object of very high C3 quality. It is located at a moderate distance from the Sun, above 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.

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
He et al. (2023) 243.921 -48.643 0.217 -2.885 -3.244 -69.26
           
UCC 243.918 -48.643 0.219 -2.885 -3.244 -69.26
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 3777 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2023) A0=6.0, m-M=13.0, logA=8.0

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
HSC 2768 88.5 243.92 -48.64 0.23 -2.88 -3.24 -69.26 0.45