CWNU 1351

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.0 0.62 0.75 0.0 0.08
C3
N_50
r_50
BA 21 1.1
Summary

CWNU 1351 is a sparse, moderately dense object of high C3 quality. It is located at a large distance from the Sun, below the mid-plane. It was recently reported in the literature.

Warning: This is very likely a duplicate object, which shares a large percentage of members with at least one previously reported entry.

Warning: contains less than 25 stars with P>0.5 estimated.

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
He et al. (2023) 201.428 -63.449 0.123 -6.952 -1.144 –
           
UCC 201.419 -63.452 0.123 -6.948 -1.136 -38.099
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 1351 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2023) A0=3.15, m-M=14.25, logAge=6.9

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
Ruprecht 166 92.0 201.42 -63.46 0.12 -6.94 -1.13 -38.1 0.5