CWNU 2835

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C3
N_50
r_50
DB 21 4.4
Summary

CWNU 2835 is a sparse, 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.

This is very likely a unique object, which shares a small percentage of members with at least one previously 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=0.76) 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) 278.346 -10.335 0.446 0.25 -0.7 26.05
           
UCC 278.358 -10.325 0.434 0.244 -0.702 26.047
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 2835 UCC

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Fundamental parameters

Reference Values
He et al. (2023) A0=4.55, m-M=11.5, logAge=9.15

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
Melotte 206 24.0 278.36 -10.4 0.47 0.03 -0.12 7.44 1.0