CWNU 95

N_50

r_50

3.5

Summary

CWNU 95 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.

Warning: This is possibly a duplicated object, which shares a significant 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. (2022)	223.296	-54.111	0.91	-2.8	-2.3	–
He et al. (2022)	223.304	-54.118	0.901	-2.806	-2.3	–
Hunt & Reffert (2023)	223.297	-54.112	0.904	-2.858	-2.311	-15.491
Cavallo et al. (2024)	222.843	-54.217	0.913	–	–	–
Hunt & Reffert (2024)	223.297	-54.112	0.904	-2.858	-2.311	-15.491

UCC	223.292	-54.102	0.909	-2.796	-2.301	-17.204

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=1.15, m-M=9.65, logAge=7.2, Z=0.002`
He et al. (2022)	`A0=1.05, logAge=7.05`
Hunt & Reffert (2023)	`AV50=1.08, diffAV50=1.408, MOD50=10.065, logAge50=7.367`
Cavallo et al. (2024)	`AV50=1.15, dMod50=10.17, logAge50=7.07, [Fe/H]50=-0.05`
Hunt & Reffert (2024)	`MassJ=184.039, MassTot=252.974`

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWWDL 14468	85.1	223.29	-54.1	0.91	-2.81	-2.31	-17.2	0.0
OC 0623	59.6	223.29	-54.1	0.91	-2.83	-2.3	-17.2	0.41