CWNU 408

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C3
N_50
r_50
BB 43 2.1
Summary

CWNU 408 is a poorly populated, very dense object of intermediate C3 quality. It is located at a moderate distance from the Sun, below the mid-plane. It was recently reported in the literature.

Warning: This is very likely a duplicate object, which shares a large percentage of members with at least one previously reported entry.

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
He et al. (2022) 126.228 -44.302 0.42 -4.56 4.48 125.2
Hunt & Reffert (2023) 126.217 -44.304 0.422 -4.589 4.5 22.909
Cavallo et al. (2024) 126.26 -44.247 0.426
Hunt & Reffert (2024) 126.217 -44.304 0.422 -4.589 4.5 22.909
           
UCC 126.215 -44.304 0.435 -4.571 4.5
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2022) AG=2.25, m-M=11.05, logAge=7.2, Z=0.002
Hunt & Reffert (2023) AV50=2.257, diffAV50=2.604, MOD50=11.613, logAge50=7.25
Cavallo et al. (2024) AV50=2.34, dMod50=11.64, logAge50=7.29, [Fe/H]50=0.25
Hunt & Reffert (2024) MassJ=838.324, MassTot=898.218

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
UBC 1442 100.0 126.21 -44.3 0.43 -4.58 4.49 0.46