CWNU 1250

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.0 0.05 0.12 0.0 1.0
C3
N_50
r_50
DC 19 61.6
Summary

CWNU 1250 is a sparse, very loose object of very low C3 quality. It is located at a very close distance from the Sun, below 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. (2022) 307.468 -30.824 2.437 3.328 -7.979 –
           
UCC 307.267 -30.775 2.131 3.03 -7.94 -5.293
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 1250 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2022) A0=0.25, logAge=9.1

Search coordinates in Bayestar19

Cluster region map