CWNU 3250

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C3
N_50
r_50
CB 22 2.1
Summary

CWNU 3250 is a sparse, very dense object of low C3 quality. It is located at a moderate distance from the Sun, above 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) 306.687 46.82 0.364 -2.027 -4.7 -8.61
           
UCC 306.687 46.82 0.377 -2.009 -4.708 -8.613
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 3250 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2023) A0=3.0, m-M=11.9, logA=7.8

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
HSC 657 92.0 306.69 46.81 0.38 -2.03 -4.72 -22.16 0.39