CWNU 47

0.41 UTI

0.46

C_N

0.24

C_dens

0.75

C_C3

0.3

C_lit

1.0

C_dup

N₅₀ (P>50% members) 46

Stellar density (N₅₀/rad) 1.2 [N/pc²]

C3 classification AB

C_N 0.46 Poorly populated
C_dens 0.24 Very loose
C_C3 0.75 High 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 47 is a poorly populated, very loose object of high C3 quality. Its parallax locates it at a relatively 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.

Relatively close Moderate extinction Near-solar metallicity Young

Cavallo et al. (2024)
Gold sample.

Data

🔍 Search references for CWNU 47 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–	301.563	23.777	0.521	-1.933	-4.722	–
Zhang et al.	2024	301.372	23.787	–	–	–	–
Hunt & Reffert	2024	301.372	23.787	0.506	-2.089	-4.78	–
Cavallo et al.	2024	301.443	23.819	0.505	–	–	–
Hunt & Reffert	2023	301.372	23.787	0.506	-2.089	-4.78	–
He et al.	2022	301.618	23.785	0.6	-1.72	-4.64	–

💡 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–	1.85	1.95	1.75	59	-0.113	125	–	–
Zhang et al.	2024	–	–	–	–	-0.113⁽¹⁾	–	–	–
Hunt & Reffert	2024	–	–	–	–	–	125⁽¹⁾	–	–
Cavallo et al.	2024	1.85	1.95	–	59	0.200	–	–	–
Hunt & Reffert	2023	1.83	1.97	1.75	74	–	–	–	–
He et al.	2022	2.34	1.50	–	3	-0.642	–	–	–

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

Visualization

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