CWNU 1618

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.0 0.14 0.25 0.0 1.0
C3
N_50
r_50
DB 22 6.7
Summary

CWNU 1618 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: 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) 317.147 47.738 0.368 -2.845 -2.787 –
           
UCC 317.181 47.752 0.352 -2.875 -2.779 –
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 1618 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2023) A0=2.55, m-M=12.0, logAge=8.65

Search coordinates in Bayestar19

Cluster region map