CWNU 3690

Click to load Aladin Lite
UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.0 0.12 0.5 0.0 1.0
C3
N_50
r_50
BB 19 2.3
Summary

CWNU 3690 is a sparse, very loose object of intermediate C3 quality. It is located at a large distance from the Sun, below the mid-plane. It was recently reported in the literature.

This object shares a large percentage of members with a later reported entry.

Warning: contains less than 25 stars with P>0.5 estimated.

Warning: the low UTI value and no obvious signs of duplication (C_dup=1.0) indicates that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
He et al. (2023) 113.635 -21.879 0.121 -1.15 1.713 –
           
UCC 113.63 -21.879 0.117 -1.142 1.719 –
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 3690 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2023) A0=2.35, m-M=13.8, logA=7.2

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
HSC 1890 80.0 113.62 -21.88 0.13 -1.17 1.75 86.6 0.09