CWNU 288

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C3
N_50
r_50
AB 22 4.2
Summary

CWNU 288 is a sparse, moderately dense object of high C3 quality. It is located at a moderate distance from the Sun, below the mid-plane. It was recently reported in the literature.

Warning: This is possibly a duplicated object, which shares a significant percentage of members with at least one previously reported entry.

Warning: contains less than 25 stars with P>0.5 estimated.

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
He et al. (2022) 98.45 -1.742 0.48 0.05 -0.84 42.1
           
UCC 98.449 -1.716 0.474 -0.068 -0.854
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 288 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2022) AG=2.0, m-M=11.65, logAge=8.1, Z=0.018

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
OC 0354 72.0 98.42 -1.72 0.47 -0.09 -0.88 24.19 0.39