CWNU 17

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.34 0.71 1.0 0.0 0.0
C3
N_50
r_50
AA 34 3.5
Summary

CWNU 17 is a poorly populated, moderately dense object of very 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 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) 56.334 50.728 0.33 0.8 -1.25 –
           
UCC 56.324 50.742 0.33 0.807 -1.247 8.411
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 17 UCC

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Fundamental parameters

Reference Values
He et al. (2022) AG=2.35, m-M=12.4, logAge=8.9, Z=0.032

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWWDL 4657 100.0 56.31 50.74 0.35 0.79 -1.25 8.41 0.0
UBC 1254 100.0 56.33 50.73 0.34 0.8 -1.25 -43.3 0.63
OC 0274 79.4 56.32 50.73 0.34 0.81 -1.26 -43.47 0.0