CWNU 4798

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.0 0.56 0.5 0.0 1.0
C3
N_50
r_50
BB 19 1.3
Summary

CWNU 4798 is a sparse, moderately dense object of intermediate C3 quality. It is located at a large distance from the Sun, below the mid-plane. It was recently reported in the literature.

This object shares a very small percentage of members with at least one entry reported in the same catalogue.

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) 247.632 -49.978 0.152 -3.367 -4.645 –
           
UCC 247.627 -49.982 0.146 -3.422 -4.641 -52.358
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 4798 UCC

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Fundamental parameters

Reference Values
He et al. (2023) A0=5.95, m-M=14.35, logA=8.9

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 4276 4.0 247.63 -50.13 0.21 -3.32 -4.15 -62.31 0.15