CWNU 1089

Click to load Aladin Lite
UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.0 0.16 0.62 0.0 0.96
C3
N_50
r_50
AC 22 16.8
Summary

CWNU 1089 is a sparse, very loose object of intermediate C3 quality. It is located at a relatively close distance from the Sun, near the mid-plane. It was recently reported in the literature.This is a unique object, which shares a very small percentage of members with at least one previously 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=0.96) 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. (2022) 80.001 35.616 0.913 -0.285 -3.21 –
           
UCC 80.072 35.626 0.924 -0.245 -3.106 -14.171
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 1089 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2022) A0=1.1, logAge=7.55

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
HSC 1341 40.0 80.52 35.48 0.94 -0.12 -3.11 -9.21 0.05
ASCC 14 4.0 80.09 35.22 0.92 -0.59 -3.65 -7.48 0.4