CWNU 1126

0.49 UTI

0.36

C_N

0.82

C_dens

0.75

C_C3

0.25

C_lit

1.0

C_dup

N₅₀ (P>50% members) 36

Stellar density (N₅₀/rad) 4.1 [N/pc²]

C3 classification AB

C_N 0.36 Poorly populated
C_dens 0.82 Dense
C_C3 0.75 High quality
C_lit 0.25 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 1126 is a poorly populated, dense object of high C3 quality. Its parallax locates it at a close distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It is poorly studied in the literature.

Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.

Close Moderate extinction Near-solar metallicity Very young

Cavallo et al. (2024)
Gold sample.

Data

🔍 Search references for CWNU 1126 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–	332.1	64.071	1.082	-1.462	-3.226	-21.606
Hunt & Reffert	2024	332.32	64.076	1.075	-1.414	-3.246	-25.15
Cavallo et al.	2024	332.186	64.095	1.073	–	–	–
Hunt & Reffert	2023	332.32	64.076	1.075	-1.414	-3.246	-25.15
He et al.	2022	332.254	64.073	1.077	-1.452	-3.22	–

💡 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–	0.965	1.06	1.4	8	0.150	126	–	–
Hunt & Reffert	2024	–	–	–	–	–	126⁽¹⁾	–	–
Cavallo et al.	2024	1.03	1.30	–	8	0.150	–	–	–
Hunt & Reffert	2023	0.90	1.06	1.40	16	–	–	–	–
He et al.	2022	–	0.90	–	8	–	–	–	–

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

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWWDL 14500	80.6	332.12	64.08	1.08	-1.49	-3.22	-20.31	0.03

💡 Note: The % column shows the percentage of members that CWNU 1126 shares with each listed object.

Visualization

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