CWNU 1111

(OCSN 120)

0.45 UTI

0.41

C_N

0.5

C_dens

0.75

C_C3

0.3

C_lit

1.0

C_dup

N₅₀ (P>50% members) 41

Stellar density (N₅₀/rad) 2.5 [N/pc²]

C3 classification AB

C_N 0.41 Poorly populated
C_dens 0.5 Moderately dense
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 1111 is a poorly populated, moderately dense object of high C3 quality. Its parallax locates it at a very close distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the absorption parameter (see Parameters). It is poorly studied in the literature.

Very close Low extinction Near-solar metallicity Young

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as a moving group.

Data

🔍 Search references for CWNU 1111 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–	85.12	13.573	3.726	-1.914	-6.025	21.855
Zhang et al.	2024	85.103	13.707	–	–	–	–
Cavallo et al.	2024	84.822	13.859	3.716	–	–	–
Hunt & Reffert	2023	85.103	13.707	3.707	-1.976	-6.105	21.523
Qin et al.	2023	84.3	14.4	3.62	-1.69	-6.4	21.21
He et al.	2022	85.181	13.382	3.745	-1.914	-6.117	–

💡 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–	0.27	0.315	0.56	22	0.007	–	–	–
Zhang et al.	2024	–	–	–	–	-0.055⁽¹⁾	–	–	–
Cavallo et al.	2024	0.27	0.78	–	21	0.070	–	–	–
Hunt & Reffert	2023	0.27	0.23	0.56	22	–	–	–	–
Qin et al.	2023	0.32	0.40	–	22	–	–	–	–
He et al.	2022	–	0.05	–	25	–	–	–	–

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

Visualization

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