CWNU 4709

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.0 0.14 0.62 0.0 0.2
C3
N_50
r_50
AC 23 18.1
Summary

CWNU 4709 is a sparse, very loose object of intermediate C3 quality. It is located at a relatively close distance from the Sun, 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) 127.9 -36.361 0.909 -5.051 4.565 20.5
           
UCC 127.912 -36.292 0.907 -5.018 4.563 21.052
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 4709 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2023) A0=0.5, m-M=10.15, logA=8.4

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
HSC 2050 80.0 128.09 -36.34 0.91 -5.02 4.55 27.82 0.23