CWNU 1490

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.3 1.0 0.25 0.33 1.0
C3
N_50
r_50
DB 30 2.8
Summary

CWNU 1490 is a poorly populated, very dense object of low 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) 313.419 47.363 0.342 -3.996 -5.404 –
Hunt & Reffert (2023) 313.393 47.344 0.337 -4.003 -5.431 -41.429
Cavallo et al. (2024) 313.393 47.361 0.338 – – –
Hunt & Reffert (2024) 313.393 47.344 0.337 -4.003 -5.431 -41.429
           
UCC 313.405 47.355 0.339 -3.994 -5.423 -30.505
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

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Estimated members

CWNU 1490 UCC
CWNU 1490 HUNT23

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Fundamental parameters

Reference Values
He et al. (2023) A0=1.3, m-M=12.4, logAge=6.65
Hunt & Reffert (2023) AV50=2.09, diffAV50=1.983, MOD50=12.201, logAge50=7.726
Cavallo et al. (2024) AV50=1.66, dMod50=12.28, logAge50=8.18, [Fe/H]50=0.99
Hunt & Reffert (2024) MassJ=309.640, MassTot=317.871

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Cluster region map