CWNU 1714

0.52 UTI

0.35

C_N

0.89

C_dens

0.75

C_C3

0.3

C_lit

1.0

C_dup

N₅₀ (P>50% members) 35

Stellar density (N₅₀/rad) 4.4 [N/pc²]

C3 classification AB

C_N 0.35 Poorly populated
C_dens 0.89 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 1714 is a poorly populated, dense object of high C3 quality. Its parallax locates it at a large distance, below the mid-plane, affected by moderate extinction. It is catalogued as a massive, near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the age parameter (see Parameters). It was recently reported in the literature.

Very distant Moderate extinction Massive Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Gold sample.

Data

🔍 Search references for CWNU 1714 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–	100.59	-1.515	0.166	-0.12	0.544	–
Hu & Soubiran	2025	100.584	-1.52	–	–	–	–
Hunt & Reffert	2024	100.595	-1.515	0.169	-0.121	0.548	87.248
Cavallo et al.	2024	100.584	-1.52	0.164	–	–	–
Hunt & Reffert	2023	100.595	-1.515	0.169	-0.121	0.548	87.248
He et al.	2023	100.596	-1.515	0.212	-0.072	0.534	–

💡 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–	5.58	1.83	2.19	223	-0.220	1278	–	–
Hu & Soubiran	2025	–	–	–	–	-0.300⁽⁵⁾	–	–	–
Hunt & Reffert	2024	–	–	–	–	–	1278⁽¹⁾	–	–
Cavallo et al.	2024	3.96	1.53	–	631	-0.140	–	–	–
Hunt & Reffert	2023	5.58	1.83	2.19	223	–	–	–	–
He et al.	2023	6.92	2.05	–	6	–	–	–	–

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

Visualization

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