CWNU 1509

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.0 0.06 0.25 0.0 1.0
C3
N_50
r_50
CC 19 9.5
Summary

CWNU 1509 is a sparse, very loose object of low C3 quality. It is located at a moderate distance from the Sun, below the mid-plane. It was recently reported in the literature.

This object shares a very small percentage of members with at least one entry reported in the same catalogue.

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) 38.405 56.754 0.354 -0.799 -0.618 –
           
UCC 38.298 56.748 0.335 -0.793 -0.623 -44.205
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 1509 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2023) A0=1.7, m-M=11.95, logAge=8.65

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 1433 4.0 37.93 56.5 0.36 -0.63 -0.48 – 0.03