CWNU 92

0.31 UTI

0.0

C_N

0.44

C_dens

0.5

C_C3

0.3

C_lit

1.0

C_dup

N₅₀ (P>50% members) 22

Stellar density (N₅₀/rad) 2.2 [N/pc²]

C3 classification BB

C_N 0.0 Sparse
C_dens 0.44 Loose
C_C3 0.5 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

ℹ️

CWNU 92 is a sparse, loose object of intermediate C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a metal-poor, young cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It is poorly studied in the literature.

Relatively close Moderate extinction Metal-poor Young

Cavallo et al. (2024)
Gold sample.

Data

🔍 Search references for CWNU 92 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	99999–	352.434	62.244	0.893	-2.342	-1.26	–
Hunt & Reffert	2024	352.402	62.229	0.88	-2.339	-1.242	–
Cavallo et al.	2024	352.408	62.237	0.888	–	–	–
Hunt & Reffert	2023	352.402	62.229	0.88	-2.339	-1.242	–
He et al.	2022	352.437	62.237	0.893	-2.331	-1.26	–
He et al.	2022	352.411	62.235	0.9	-2.33	-1.26	–

💡 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–	1.08	2.705	1.0	38	-0.854	147	–	–
Hunt & Reffert	2024	–	–	–	–	–	147⁽¹⁾	–	–
Cavallo et al.	2024	1.09	2.59	–	43	0.320	–	–	–
Hunt & Reffert	2023	1.08	2.40	1.00	60	–	–	–	–
He et al.	2022	–	2.85	–	28	–	–	–	–
He et al.	2022	0.89	2.82	–	32	-2.028	–	–	–

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

Visualization

ℹ️

1 2