CWNU 3636

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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 20 1.5
Summary

CWNU 3636 is a sparse, very loose object of intermediate C3 quality. It is located at a very large distance from the Sun, well 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) 124.716 -44.781 0.062 -1.687 2.517 107.34
           
UCC 124.697 -44.742 0.082 -1.75 2.561 107.344
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 3636 UCC

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2023) A0=2.05, m-M=14.45, logA=8.8

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
HSC 2100 80.0 124.7 -44.74 0.08 -1.73 2.62 104.5 0.11