CWNU 3790

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.0 1.0 0.75 0.0 0.2
C3
N_50
r_50
AB 22 1.0
Summary

CWNU 3790 is a sparse, very dense object of high C3 quality. It is located at a large 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) 85.693 25.277 0.208 0.553 -0.103 –
           
UCC 85.691 25.278 0.196 0.554 -0.103 –
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 3790 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2023) A0=2.65, m-M=14.0, logA=8.0

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
HSC 1443 80.0 85.69 25.28 0.2 0.62 -0.12 – 0.48