CWNU 4474

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C3
N_50
r_50
BB 18 7.1
Summary

CWNU 4474 is a sparse, very loose object of intermediate C3 quality. It is located at a large distance from the Sun, well above the mid-plane. It was recently reported in the literature.

Warning: This is 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) 116.773 -16.128 0.147 -1.391 1.567 86.09
           
UCC 116.759 -16.094 0.14 -1.394 1.555 86.085
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 4474 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2023) A0=1.8, m-M=15.35, logA=8.3

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
HSC 1846 80.0 116.76 -16.17 0.13 -1.4 1.55 86.09 0.1