CWNU 1760

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.0 0.61 0.12 0.33 1.0
C3
N_50
r_50
DC 24 4.9
Summary

CWNU 1760 is a sparse, moderately dense object of very low C3 quality. It is located at a relatively close distance from the Sun, near the mid-plane. It was recently reported in the literature.

Warning: contains less than 25 stars with P>0.5 estimated.

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
He et al. (2023) 66.465 48.743 0.518 0.168 -2.395 -28.06
Hunt & Reffert (2023) 66.482 48.762 0.517 0.132 -2.359 115.844
Cavallo et al. (2024) 66.478 48.725 0.516 – – –
Hunt & Reffert (2024) 66.482 48.762 0.517 0.132 -2.359 115.844
           
UCC 66.465 48.735 0.509 0.168 -2.391 90.298
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

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Estimated members

CWNU 1760 UCC
CWNU 1760 HUNT23

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Fundamental parameters

Reference Values
He et al. (2023) A0=4.15, m-M=11.55, logAge=8.65
Hunt & Reffert (2023) AV50=3.552, diffAV50=2.275, MOD50=11.34, logAge50=8.292
Cavallo et al. (2024) AV50=3.97, dMod50=12.27, logAge50=7.82, [Fe/H]50=0.04
Hunt & Reffert (2024) MassJ=153.689, MassTot=153.689

Search coordinates in Bayestar19

Cluster region map