CWNU 180

0.25 UTI

0.0

C_N

0.27

C_dens

0.38

C_C3

0.3

C_lit

1.0

C_dup

N₅₀ (P>50% members) 23

Stellar density (N₅₀/rad) 1.3 [N/pc²]

C3 classification CB

C_N 0.0 Sparse
C_dens 0.27 Loose
C_C3 0.38 Low 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 180 is a sparse, loose object of low C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a very metal-poor, young cluster, but with a large variance across recent sources for the absorption, age, and metallicity parameters (see Parameters). It is poorly studied in the literature.

Relatively close Moderate extinction Very metal-poor Young

Cavallo et al. (2024)
Gold sample.

Data

🔍 Search references for CWNU 180 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–	307.7	38.101	0.964	-1.572	-3.899	4.463
Hunt & Reffert	2024	307.555	38.173	0.932	-1.599	-3.908	-5.817
Cavallo et al.	2024	307.686	38.104	0.943	–	–	–
Hunt & Reffert	2023	307.555	38.173	0.932	-1.599	-3.908	-5.817
He et al.	2022	307.78	38.367	0.971	-1.572	-3.885	–
He et al.	2022	307.901	37.839	0.96	-1.6	-3.98	–

💡 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–	1.1	1.795	2.31	26	-1.009	109	–	–
Hunt & Reffert	2024	–	–	–	–	–	109⁽¹⁾	–	–
Cavallo et al.	2024	1.11	2.06	–	28	0.010	–	–	–
Hunt & Reffert	2023	1.00	1.64	2.31	24	–	–	–	–
He et al.	2022	–	1.95	–	32	–	–	–	–
He et al.	2022	1.10	0.24	–	2	-2.028	–	–	–

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

Visualization

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