CWNU 3770

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.0 0.24 0.25 0.0 0.16
C3
N_50
r_50
CC 23 9.2
Summary

CWNU 3770 is a sparse, very loose object of low C3 quality. It is located at a relatively close distance from the Sun, near 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) 110.251 -19.448 0.61 -3.084 1.938 58.15
           
UCC 110.242 -19.416 0.61 -3.071 1.961 53.233
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 3770 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2023) A0=0.75, m-M=11.0, logA=8.4

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
HSC 1844 84.0 110.26 -19.43 0.61 -3.09 1.95 53.23 0.09