CWNU 3290

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C3
N_50
r_50
BA 43 1.5
Summary

CWNU 3290 is a poorly populated, very dense object of high C3 quality. It is located at a large distance from the Sun, above 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. (2023) 90.253 32.009 0.187 0.917 -1.103 10.94
           
UCC 90.253 32.009 0.169 0.928 -1.116 10.936
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 3290 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2023) A0=2.4, m-M=13.35, logA=8.4

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
HSC 1413 90.7 90.26 32.01 0.18 0.91 -1.1 10.94 0.59