CWNU 1406

0.23 UTI

0.0

C_N

0.27

C_dens

0.75

C_C3

0.06

C_lit

1.0

C_dup

N_m (P>50%) 23

Core radius and density 1.3 [pc], 1.4 [pc^-2]

C3 classification AB

C_N 0.0 Sparse
C_dens 0.27 Loose
C_C3 0.75 High quality
C_lit 0.06 Rarely studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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CWNU 1406 is a sparse, loose object of high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by high extinction. It is catalogued as a metal-rich, very young cluster (see Parameters). It was recently reported in the literature.

⚠️ Warning: the low UTI value and no obvious signs of duplication (C_dup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Relatively close High extinction Metal-rich Very young

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.77 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.77 (50th percentile).

Data

🔍 Search references for CWNU 1406 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–	47.838	55.175	0.406	-0.318	-0.619	–
Hunt & Reffert	2024	47.827	55.202	0.4	-0.307	-0.649	–
Cavallo et al.	2024	47.801	55.188	0.4	–	–	–
Hunt & Reffert	2023	47.827	55.202	0.4	-0.307	-0.649	–
He et al.	2023	47.816	55.204	0.415	-0.335	-0.636	–

💡 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–	2.405	3.95	2.67	18	0.680	441	–	–
Hunt & Reffert	2024	2.24	3.95	2.67	24	–	441⁽¹⁾	–	–
Cavallo et al.	2024	2.73	3.62	–	12	0.680	–	–	–
Hunt & Reffert	2023	2.24	3.95	2.67	24	–	–	–	–
He et al.	2023	2.57	4.50	–	8	–	–	–	–

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

Visualization

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