CWNU 409

UTI: UCC Trust Index C_N C_dens C_C3 C_lit C_dup 0.42 1.0 0.75 0.42 1.0
C3	N_50	r_50
AB	42	7.2

Summary

CWNU 409 is a poorly populated, very dense object of high C3 quality. It is located at a relatively close distance from the Sun, above the mid-plane. It was recently reported in the literature.

Search object in SciX | Simbad

Positions

Reference	RA	DEC	Plx	pmRA	pmDE	Rv
He et al. (2022)	69.023	59.75	0.96	-0.79	-1.43	–
He et al. (2022)	69.0	59.718	0.956	-0.687	-1.55	–
Hunt & Reffert (2023)	69.007	59.735	0.961	-0.802	-1.473	-16.03
Cavallo et al. (2024)	69.048	59.74	0.974	–	–	–
Hunt & Reffert (2024)	69.007	59.735	0.961	-0.802	-1.473	-16.03
UCC	69.017	59.748	0.955	-0.8	-1.517	-16.376

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. (2022)	AG=1.7, m-M=10.25, logAge=7.0, Z=0.014
He et al. (2022)	A0=1.75, logAge=8.7
Hunt & Reffert (2023)	AV50=1.262, diffAV50=0.747, MOD50=9.955, logAge50=7.159
Cavallo et al. (2024)	AV50=1.54, dMod50=10.31, logAge50=6.86, [Fe/H]50=0.26
Hunt & Reffert (2024)	MassJ=96.6676, MassTot=146.675

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Cluster region map