CWNU 1718

N_50

r_50

7.1

Summary

CWNU 1718 is a poorly populated, loose object of very low C3 quality. It is located at a moderate distance from the Sun, above the mid-plane. It was recently reported in the literature.

This is likely a unique object, which shares a moderate percentage of members with at least one previously reported entry.

Search object in SciX | Simbad

Positions

Reference	RA	DEC	Plx	pmRA	pmDE	Rv
He et al. (2023)	84.839	32.555	0.484	-0.28	-1.4	–
Hunt & Reffert (2023)	84.805	32.609	0.478	-0.27	-1.392	–
Cavallo et al. (2024)	84.827	32.542	0.475	–	–	–
Hunt & Reffert (2024)	84.805	32.609	0.478	-0.27	-1.392	–
Zhang et al. (2024)	84.805	32.609	–	–	–	–

UCC	84.808	32.599	0.482	-0.257	-1.4	–

Galactocentric position

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

1 2

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Fundamental parameters

Reference	Values
He et al. (2023)	`A0=1.7, m-M=11.8, logAge=7.05`
Hunt & Reffert (2023)	`AV50=1.56, diffAV50=1.883, MOD50=11.485, logAge50=8.247`
Cavallo et al. (2024)	`AV50=1.7, dMod50=11.78, logAge50=7.93, [Fe/H]50=0.4`
Hunt & Reffert (2024)	`MassJ=220.249, MassTot=239.137`
Zhang et al. (2024)	`[Fe/H]ANN=-0.0993, [Fe/H]MCMC=-0.0895`

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Teutsch J0538.2+3234	36.0	84.57	32.6	0.33	-0.22	-1.48	38.83	0.06