CWNU 2490

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.26 1.0 0.62 0.33 1.0
C3
N_50
r_50
AC 26 1.3
Summary

CWNU 2490 is a poorly populated, very dense object of intermediate C3 quality. It is located at a moderate distance from the Sun, above the mid-plane. It was recently reported in the literature.

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Positions

Reference RA DEC Plx pmRA pmDE Rv
He et al. (2023) 58.991 55.337 0.321 -0.449 -0.73 –
Hunt & Reffert (2023) 58.992 55.335 0.296 -0.442 -0.717 –
Cavallo et al. (2024) 59.003 55.356 0.309 – – –
Hunt & Reffert (2024) 58.992 55.335 0.296 -0.442 -0.717 –
           
UCC 58.989 55.336 0.323 -0.446 -0.727 –
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

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Estimated members

CWNU 2490 UCC
CWNU 2490 HUNT23

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Fundamental parameters

Reference Values
He et al. (2023) A0=2.65, m-M=12.35, logAge=8.05
Hunt & Reffert (2023) AV50=2.467, diffAV50=0.999, MOD50=12.37, logAge50=8.042
Cavallo et al. (2024) AV50=2.79, dMod50=12.31, logAge50=7.68, [Fe/H]50=-0.4
Hunt & Reffert (2024) MassJ=219.177, MassTot=246.731

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Cluster region map