CWNU 168

0.34 UTI

0.25

C_N

0.22

C_dens

0.62

C_C3

0.3

C_lit

1.0

C_dup

N₅₀ (P>50% members) 25

Stellar density (N₅₀/rad) 1.1 [N/pc²]

C3 classification AC

C_N 0.25 Poorly populated
C_dens 0.22 Very loose
C_C3 0.62 Intermediate quality
C_lit 0.3 Poorly studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

MOCA 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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CWNU 168 is a poorly populated, very loose object of intermediate C3 quality. Its parallax locates it at a close distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the age and metallicity parameters (see Parameters). It is poorly studied in the literature.

Close Moderate extinction Near-solar metallicity Young

Cavallo et al. (2024)
Gold sample.

Data

🔍 Search references for CWNU 168 in: SciX Simbad

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Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	99999–	81.066	20.731	1.213	-0.138	-4.657	-7.162
Zhang et al.	2024	81.067	20.723	–	–	–	–
Hunt & Reffert	2024	81.067	20.723	1.206	-0.126	-4.651	-16.872
Cavallo et al.	2024	80.997	20.684	1.203	–	–	–
Hunt & Reffert	2023	81.067	20.723	1.206	-0.126	-4.651	-16.872
He et al.	2022	80.862	20.662	1.2	-0.21	-4.67	–

💡 Note: The UCC values are estimated from its identified members.

Reference	Year	Dist [kpc]	Av [mag]	DAv [mag]	Age [Myr]	[Fe/H] [dex]	Mass [Msun]	B_frac	BSS
UCC	99999–	0.85	1.14	0.46	23	0.370	77	–	–
Zhang et al.	2024	–	–	–	–	-0.148⁽¹⁾	–	–	–
Hunt & Reffert	2024	–	–	–	–	–	77⁽¹⁾	–	–
Cavallo et al.	2024	0.91	1.16	–	19	0.370	–	–	–
Hunt & Reffert	2023	0.78	0.96	0.46	23	–	–	–	–
He et al.	2022	0.85	1.14	–	158	0.916	–	–	–

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Visualization

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