CWNU 1892

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C3
N_50
r_50
CC 21 9.2
Summary

CWNU 1892 is a sparse, very loose object of low C3 quality. It is located at a relatively close distance from the Sun, below 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) 125.408 -43.712 0.618 -4.588 4.136
           
UCC 125.398 -43.661 0.618 -4.584 4.136 18.975
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 1892 UCC

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Fundamental parameters

Reference Values
He et al. (2023) A0=2.1, m-M=11.15, logAge=7.95

Search coordinates in Bayestar19

Cluster region map