CWNU 2180

UTI: UCC Trust Index C_N C_dens C_C3 C_lit C_dup 0.0 0.24 0.12 0.33 1.0
C3	N_50	r_50
DC	24	11.9

Summary

CWNU 2180 is a sparse, very loose 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)	83.117	30.565	0.777	-1.264	-4.225	–
Hunt & Reffert (2023)	83.15	30.602	0.773	-1.22	-4.235	-20.94
Cavallo et al. (2024)	83.078	30.655	0.773	–	–	–
Hunt & Reffert (2024)	83.15	30.602	0.773	-1.22	-4.235	-20.94
UCC	83.138	30.578	0.775	-1.262	-4.217	-21.013

Galactocentric position

How are the galactocentric plots generated?

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Estimated members

1 2

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Fundamental parameters

Reference	Values
He et al. (2023)	A0=2.0, m-M=10.65, logAge=8.4
Hunt & Reffert (2023)	AV50=1.696, diffAV50=0.644, MOD50=10.494, logAge50=8.133
Cavallo et al. (2024)	AV50=1.89, dMod50=10.6, logAge50=8.35, [Fe/H]50=0.24
Hunt & Reffert (2024)	MassJ=71.9567, MassTot=111.240

Search coordinates in Bayestar19

Cluster region map