CWNU 3499

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C3
N_50
r_50
AC 19 3.0
Summary

CWNU 3499 is a sparse, very loose object of intermediate C3 quality. It is located at a very large distance from the Sun, well above the mid-plane. It was recently reported in the literature.

Warning: This is possibly a duplicated object, which shares a significant 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) 336.098 64.537 0.1 -1.974 -1.008
           
UCC 336.094 64.541 0.095 -2.014 -1.056 -101.778
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 3499 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2023) A0=3.2, m-M=14.45, logA=8.9

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
HSC 841 56.0 336.02 64.54 0.09 -1.98 -1.05 -101.78 0.22