CWNU 2619

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.54 1.0 1.0 0.33 0.96
C3
N_50
r_50
AA 57 1.8
Summary

CWNU 2619 is a moderately populated, very dense 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 is a unique object, which shares a very small percentage of members with at least one previously reported entry.

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Positions

Reference RA DEC Plx pmRA pmDE Rv
He et al. (2023) 314.903 44.967 0.326 -3.57 -4.558 –
Hunt & Reffert (2023) 314.901 44.97 0.317 -3.57 -4.551 -27.336
Cavallo et al. (2024) 314.891 44.955 0.316 – – –
Hunt & Reffert (2024) 314.901 44.97 0.317 -3.57 -4.551 -27.336
           
UCC 314.902 44.964 0.321 -3.571 -4.559 -27.32
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

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Estimated members

CWNU 2619 UCC
CWNU 2619 HUNT23

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Fundamental parameters

Reference Values
He et al. (2023) A0=2.45, m-M=12.55, logAge=7.2
Hunt & Reffert (2023) AV50=1.962, diffAV50=1.56, MOD50=12.313, logAge50=7.986
Cavallo et al. (2024) AV50=1.92, dMod50=12.35, logAge50=8.58, [Fe/H]50=0.13
Hunt & Reffert (2024) MassJ=383.052, MassTot=383.052

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
FoF 341 3.5 314.9 44.93 0.27 -3.4 -4.4 -33.82 0.03