CWNU 3789

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.0 0.57 0.75 0.0 0.12
C3
N_50
r_50
AB 22 6.3
Summary

CWNU 3789 is a sparse, moderately dense object of high 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) 89.144 27.639 0.653 0.149 -2.3 –
           
UCC 89.138 27.642 0.658 0.141 -2.301 27.49
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 3789 UCC

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Fundamental parameters

Reference Values
He et al. (2023) A0=1.65, m-M=10.85, logA=7.2

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
HSC 1440 88.0 89.16 27.64 0.65 0.14 -2.3 27.49 0.45