CWNU 1257

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.0 0.14 0.75 0.0 1.0
C3
N_50
r_50
AB 24 41.2
Summary

CWNU 1257 is a sparse, very loose object of high C3 quality. It is located at a very close distance from the Sun, above the mid-plane. It was recently reported in the literature.

This object shares a 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. (2022) 298.113 41.218 2.035 1.549 -0.221 –
           
UCC 298.614 41.441 2.045 1.507 -0.227 -9.305
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 1257 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2022) A0=0.6, logAge=7.5

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
Theia 540 12.0 296.62 39.82 2.11 1.47 -0.65 -9.9 0.16