CWNU 338

Click to load Aladin Lite
UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.74 1.0 1.0 0.42 0.75
C3
N_50
r_50
AA 99 17.9
Summary

CWNU 338 is a moderately populated, very dense object of very high C3 quality. It is located at a close distance from the Sun, near the mid-plane. It was recently reported in the literature.

This is very likely a unique object, which shares a small 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) 124.499 -39.285 1.59 -5.25 5.4 36.9
He et al. (2022) 124.472 -39.302 1.61 -5.249 5.47 –
Hunt & Reffert (2023) 124.443 -39.329 1.61 -5.385 5.352 24.205
Cavallo et al. (2024) 125.062 -38.451 1.612 – – –
Hunt & Reffert (2024) 124.443 -39.329 1.61 -5.385 5.352 24.205
           
UCC 124.556 -39.251 1.594 -5.242 5.425 30.762
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 338 UCC
CWNU 338 HUNT23

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2022) AG=0.45, m-M=8.85, logAge=7.2, Z=0.018
He et al. (2022) A0=1.0, logAge=7.15
Hunt & Reffert (2023) AV50=0.317, diffAV50=0.885, MOD50=8.856, logAge50=7.015
Cavallo et al. (2024) AV50=0.69, dMod50=9.02, logAge50=6.72, [Fe/H]50=-0.11
Hunt & Reffert (2024) MassJ=50.4718, MassTot=128.549

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
OC 0451 25.3 124.53 -39.23 1.62 -5.25 5.51 26.33 0.35