CWNU 4792

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.0 0.03 0.38 0.0 1.0
C3
N_50
r_50
BC 14 4.7
Summary

CWNU 4792 is a sparse, very loose object of low C3 quality. It is located at a large distance from the Sun, above the mid-plane. It was recently reported in the literature.

This object shares a significant percentage of members with a later reported entry.

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) 276.849 -2.424 0.106 -2.12 -4.944 –
           
UCC 276.845 -2.408 0.14 -2.164 -4.946 –
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 4792 UCC

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Fundamental parameters

Reference Values
He et al. (2023) A0=3.4, m-M=16.1, logA=9.1

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
HSC 280 52.0 276.85 -2.41 0.16 -2.16 -4.75 58.43 0.01