CWNU 1137

0.46 UTI

0.38

C_N

0.66

C_dens

0.75

C_C3

0.25

C_lit

1.0

C_dup

N₅₀ (P>50% members) 38

Stellar density (N₅₀/rad) 3.3 [N/pc²]

C3 classification BA

C_N 0.38 Poorly populated
C_dens 0.66 Moderately 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 1137 is a poorly populated, moderately dense object of high C3 quality. Its parallax locates it at a close distance, above the mid-plane, affected by low extinction. It is catalogued as a metal-rich, intermediate-age cluster (see Parameters). It is poorly studied in the literature.

Close Low extinction Metal-rich Intermediate age

Cavallo et al. (2024)
Gold sample.

Data

🔍 Search references for CWNU 1137 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–	66.851	58.371	1.466	-1.335	-1.465	-6.16
Hunt & Reffert	2024	66.831	58.357	1.472	-1.338	-1.479	-7.542
Cavallo et al.	2024	66.744	58.493	1.472	–	–	–
Hunt & Reffert	2023	66.831	58.357	1.472	-1.338	-1.479	-7.542
He et al.	2022	66.986	58.343	1.481	-1.326	-1.443	–

💡 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–	0.69	0.86	0.82	112	0.530	63	–	–
Hunt & Reffert	2024	–	–	–	–	–	63⁽¹⁾	–	–
Cavallo et al.	2024	0.73	0.86	–	151	0.530	–	–	–
Hunt & Reffert	2023	0.65	0.69	0.82	79	–	–	–	–
He et al.	2022	–	0.95	–	112	–	–	–	–

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

Visualization

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