CWNU 216

(OCSN 150)

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C3
N_50
r_50
AA 26 7.3
Summary

CWNU 216 is a poorly populated, very dense object of very high C3 quality. It is located at a very close distance from the Sun, below the mid-plane. It was recently reported in the literature.

Warning: This is very 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) 79.44 7.195 2.54 2.23 -3.71 15.2
He et al. (2022) 79.427 7.213 2.539 2.33 -3.697
Qin et al. (2023) 79.42 7.16 2.54 2.34 -3.71 0.45
           
UCC 79.419 7.169 2.539 2.219 -3.705 14.328
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 216 UCC

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Fundamental parameters

Reference Values
He et al. (2022) AG=1.15, m-M=7.6, logAge=6.5, Z=0.004
He et al. (2022) A0=0.1, logAge=6.5
Qin et al. (2023) E(B-V)=0.37, m-M=9.13, logt=6.7

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
OC 0322 96.2 79.44 7.18 2.54 2.23 -3.7 11.82 0.56