CWNU 4495

Click to load Aladin Lite
UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.0 0.04 0.12 0.0 1.0
C3
N_50
r_50
DC 15 6.0
Summary

CWNU 4495 is a sparse, very loose object of very low C3 quality. It is located at a large distance from the Sun, above the mid-plane. It was recently reported in the literature.

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) 76.758 49.246 0.201 0.446 -0.67 –
           
UCC 76.709 49.215 0.199 0.449 -0.632 -42.393
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 4495 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2023) A0=1.35, m-M=13.1, logA=9.4

Search coordinates in Bayestar19

Cluster region map