CWNU 1700

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C3
N_50
r_50
CB 20 3.0
Summary

CWNU 1700 is a sparse, loose object of low C3 quality. It is located at a moderate distance from the Sun, below 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) 291.73 13.953 0.285 -3.074 -5.884
           
UCC 291.732 13.952 0.276 -3.071 -5.889 59.282
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 1700 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2023) A0=5.85, m-M=13.1, logAge=6.3

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
FSR 0129 80.0 291.73 13.95 0.28 -3.06 -5.88 59.28 0.34