CWNU 1790

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.3 1.0 0.62 0.33 1.0
C3
N_50
r_50
AC 30 5.3
Summary

CWNU 1790 is a poorly populated, very dense object of intermediate C3 quality. It is located at a relatively close distance from the Sun, near 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) 327.234 53.905 0.642 -4.558 -6.222 –
Hunt & Reffert (2023) 327.198 53.875 0.605 -4.636 -6.237 -78.567
Cavallo et al. (2024) 327.242 53.909 0.628 – – –
Hunt & Reffert (2024) 327.198 53.875 0.605 -4.636 -6.237 -78.567
           
UCC 327.235 53.914 0.634 -4.571 -6.222 –
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

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Estimated members

CWNU 1790 UCC
CWNU 1790 HUNT23

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Fundamental parameters

Reference Values
He et al. (2023) A0=1.8, m-M=10.95, logAge=8.4
Hunt & Reffert (2023) AV50=1.786, diffAV50=1.563, MOD50=10.882, logAge50=8.585
Cavallo et al. (2024) AV50=1.76, dMod50=11.24, logAge50=8.46, [Fe/H]50=0.2
Hunt & Reffert (2024) MassJ=157.198, MassTot=179.432

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Cluster region map