CWNU 2017

Click to load Aladin Lite
UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.25 0.14 0.75 0.0 1.0
C3
N_50
r_50
AB 25 10.9
Summary

CWNU 2017 is a poorly populated, very loose object of high C3 quality. It is located at a relatively close distance from the Sun, above the mid-plane. It was recently reported in the literature.

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

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) 90.128 27.614 0.537 -0.222 -2.234 9.9
           
UCC 90.15 27.572 0.532 -0.222 -2.243 9.895
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 2017 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2023) A0=0.85, m-M=11.25, logAge=7.45

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
HSC 1445 48.0 90.29 27.22 0.51 -0.22 -2.29 -33.01 0.14