CWNU 2413

0.43 UTI

0.39

C_N

0.43

C_dens

0.75

C_C3

0.3

C_lit

1.0

C_dup

N₅₀ (P>50% members) 39

Stellar density (N₅₀/rad) 2.2 [N/pc²]

C3 classification AB

C_N 0.39 Poorly populated
C_dens 0.43 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 2413 is a poorly populated, loose object of high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It was recently reported in the literature.

Relatively close Low extinction Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Gold sample.

Data

🔍 Search references for CWNU 2413 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–	160.385	-56.6	0.438	-7.815	3.426	-10.708
Hu & Soubiran	2025	160.423	-56.614	–	–	–	–
Hunt & Reffert	2024	160.347	-56.639	0.436	-7.855	3.442	7.778
Cavallo et al.	2024	160.423	-56.614	0.435	–	–	–
Hunt & Reffert	2023	160.347	-56.639	0.436	-7.855	3.442	7.778
He et al.	2023	160.519	-56.598	0.435	-7.805	3.414	–

💡 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–	2.11	0.86	1.2	447	0.060	151	–	–
Hu & Soubiran	2025	–	–	–	–	-0.120⁽⁵⁾	–	–	–
Hunt & Reffert	2024	–	–	–	–	–	151⁽¹⁾	–	–
Cavallo et al.	2024	2.11	0.80	–	513	0.240	–	–	–
Hunt & Reffert	2023	2.09	0.86	1.20	328	–	–	–	–
He et al.	2023	2.14	1.05	–	447	–	–	–	–

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

Visualization

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