CWNU 3890

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.0 0.7 0.12 0.0 1.0
C3
N_50
r_50
DC 22 1.7
Summary

CWNU 3890 is a sparse, moderately dense object of very low C3 quality. It is located at a large 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) 98.716 6.67 0.199 -0.076 0.271 –
           
UCC 98.716 6.675 0.198 -0.085 0.313 –
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 3890 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2023) A0=3.1, m-M=14.05, logA=7.2

Search coordinates in Bayestar19

Cluster region map