CWNU 1717

Click to load Aladin Lite
C3
N_50
r_50
AA 29 4.3
Summary

CWNU 1717 is a poorly populated, loose object of very high 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 significant 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) 271.227 -21.243 0.284 -0.792 -1.967
Hunt & Reffert (2023) 271.077 -21.22 0.265 -0.777 -1.942 6.42
Cavallo et al. (2024) 271.152 -21.242 0.266
Hunt & Reffert (2024) 271.077 -21.22 0.265 -0.777 -1.942 6.42
           
UCC 271.157 -21.219 0.266 -0.795 -1.948 3.337
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=4.85, m-M=12.9, logAge=6.55
Hunt & Reffert (2023) AV50=4.318, diffAV50=2.743, MOD50=12.817, logAge50=7.077
Cavallo et al. (2024) AV50=4.54, dMod50=11.53, logAge50=6.88, [Fe/H]50=-0.78
Hunt & Reffert (2024) MassJ=1407.18, MassTot=1791.33

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWWL 2457 55.2 271.07 -21.24 0.27 -0.75 -1.93 11.39 0.22