CWNU 1394

Click to load Aladin Lite
C3
N_50
r_50
DB 52 3.4
Summary

CWNU 1394 is a moderately populated, very dense object of low C3 quality. It is located at a moderate distance from the Sun, near the mid-plane. It was recently reported in the literature.

This object shares a large percentage of members with a later reported entry.

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
He et al. (2023) 141.318 -52.332 0.397 -5.741 5.401 6.29
Hunt & Reffert (2023) 141.314 -52.331 0.385 -5.712 5.402 34.103
Cavallo et al. (2024) 141.31 -52.341 0.391
Hunt & Reffert (2024) 141.314 -52.331 0.385 -5.712 5.402 34.103
           
UCC 141.303 -52.339 0.389 -5.731 5.413 34.077
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. (2023) A0=1.9, m-M=12.0, logAge=8.8
Hunt & Reffert (2023) AV50=1.868, diffAV50=1.707, MOD50=11.824, logAge50=8.648
Cavallo et al. (2024) AV50=1.78, dMod50=12.27, logAge50=8.62, [Fe/H]50=0.62
Hunt & Reffert (2024) MassJ=295.459, MassTot=317.394

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWWDL 4995 76.9 141.31 -52.34 0.41 -5.74 5.4 6.29 0.01