CWNU 4777

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C3
N_50
r_50
BC 21 5.2
Summary

CWNU 4777 is a sparse, very loose 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) 87.362 27.66 0.21 0.496 -0.032 25.27
           
UCC 87.361 27.7 0.213 0.492 -0.031 25.271
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 4777 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2023) A0=2.4, m-M=13.15, logA=9.0

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
HSC 1431 76.0 87.36 27.62 0.2 0.51 -0.06 25.27 0.07