CWNU 317

Click to load Aladin Lite
UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.46 1.0 1.0 0.33 1.0
C3
N_50
r_50
AA 46 4.0
Summary

CWNU 317 is a poorly populated, very dense object of very high C3 quality. It is located at a relatively close distance from the Sun, above the mid-plane. It was recently reported in the literature.

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
He et al. (2022) 254.143 -39.828 0.65 -1.81 -2.25 -9.5
Hunt & Reffert (2023) 254.163 -39.848 0.69 -1.752 -2.297 -39.629
Cavallo et al. (2024) 254.175 -39.869 0.689 – – –
Hunt & Reffert (2024) 254.163 -39.848 0.69 -1.752 -2.297 -39.629
           
UCC 254.17 -39.859 0.687 -1.783 -2.307 -47.349
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 317 UCC
CWNU 317 HUNT23

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2022) AG=1.05, m-M=11.0, logAge=8.4, Z=0.04
Hunt & Reffert (2023) AV50=1.203, diffAV50=0.524, MOD50=10.676, logAge50=8.106
Cavallo et al. (2024) AV50=1.59, dMod50=10.66, logAge50=7.83, [Fe/H]50=0.17
Hunt & Reffert (2024) MassJ=214.190, MassTot=217.546

Search coordinates in Bayestar19

Cluster region map