CWNU 2352

Click to load Aladin Lite
UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.31 1.0 1.0 0.33 0.97
C3
N_50
r_50
AA 31 2.1
Summary

CWNU 2352 is a poorly populated, very dense object of very high C3 quality. It is located at a moderate distance from the Sun, below the mid-plane. It was recently reported in the literature.This is a unique object, which shares a very 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. (2023) 35.346 58.011 0.296 -1.335 -0.39 -53.69
Hunt & Reffert (2023) 35.389 57.998 0.287 -1.337 -0.414 –
Cavallo et al. (2024) 35.353 57.997 0.287 – – –
Hunt & Reffert (2024) 35.389 57.998 0.287 -1.337 -0.414 –
           
UCC 35.375 57.994 0.287 -1.339 -0.418 –
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

CWNU 2352 UCC
CWNU 2352 HUNT23

Explore data in Colab

Fundamental parameters

Reference Values
He et al. (2023) A0=2.35, m-M=12.45, logAge=8.15
Hunt & Reffert (2023) AV50=2.181, diffAV50=0.674, MOD50=12.478, logAge50=8.0
Cavallo et al. (2024) AV50=2.43, dMod50=12.77, logAge50=7.82, [Fe/H]50=0.04
Hunt & Reffert (2024) MassJ=321.032, MassTot=343.317

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
FoF 921 3.2 35.61 58.0 0.26 -1.04 -0.37 -37.7 0.03