CWNU 4770

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.0 0.14 0.38 0.0 1.0
C3
N_50
r_50
BC 23 18.2
Summary

CWNU 4770 is a sparse, very loose 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: 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) 77.998 33.963 0.933 -0.752 -3.253 –
           
UCC 77.998 33.965 0.932 -0.714 -3.241 -10.4
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 4770 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2023) A0=0.05, m-M=10.2, logA=7.0

Search coordinates in Bayestar19

Cluster region map