CWNU 390

Click to load Aladin Lite
UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.41 1.0 0.75 0.0 0.12
C3
N_50
r_50
AB 41 4.2
Summary

CWNU 390 is a poorly populated, very dense object of high C3 quality. It is located at a relatively close distance from the Sun, below 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) 68.718 38.392 0.61 0.58 -3.23 -15.7
           
UCC 68.7 38.397 0.599 0.587 -3.225 -15.713
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 390 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2022) AG=1.8, m-M=10.5, logAge=9.0, Z=0.004

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
UBC 1272 87.8 68.7 38.4 0.6 0.59 -3.23 -15.71 0.56