CWNU 492

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C3
N_50
r_50
AB 83 8.4
Summary

CWNU 492 is a moderately populated, very dense object of high C3 quality. It is located at a close distance from the Sun, above the mid-plane. It was recently reported in the literature.

Warning: This is likely a duplicate object, which shares a large percentage of members with at least one previously reported entry.

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
He et al. (2022) 278.655 -1.851 1.15 -2.2 -3.07
He et al. (2022) 278.659 -1.841 1.153 -2.195 -3.049
           
UCC 278.68 -1.858 1.124 -2.198 -3.058 -40.736
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 492 UCC

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Fundamental parameters

Reference Values
He et al. (2022) AG=4.3, m-M=9.15, logAge=8.9, Z=0.014
He et al. (2022) A0=4.1, logAge=6.0

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
OC 0056 80.7 278.68 -1.86 1.13 -2.2 -3.06 -40.74 0.47
UPK 34 77.1 278.67 -1.86 1.13 -2.2 -3.06 -40.74 0.03