CWNU 2714

0.41 UTI

0.55

C_N

0.6

C_dens

0.75

C_C3

0.06

C_lit

1.0

C_dup

N_m (P>50%) 59

Core radius and density 1.1 [pc], 3.0 [pc^-2]

C3 classification AB

C_N 0.55 Moderately populated
C_dens 0.6 Moderately dense
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 2714 is a moderately populated, moderately dense object of high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a metal-rich, young cluster, but with a large variance across recent sources for the age parameter (see Parameters). It was recently reported in the literature.

Relatively close Moderate extinction Metal-rich Young

Palma et al. (2025)
Part of multiple system G57, along with CWNU_2606 and CWNU_62.

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.96 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.96 (50th percentile).

Data

🔍 Search references for CWNU 2714 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–	256.927	-42.645	0.621	1.069	-1.811	-35.031
Hunt & Reffert	2024	256.917	-42.649	0.617	1.043	-1.864	-25.466
Cavallo et al.	2024	256.852	-42.676	0.618	–	–	–
Hunt & Reffert	2023	256.917	-42.649	0.617	1.043	-1.864	-25.466
He et al.	2023	256.91	-42.635	0.622	1.076	-1.803	-26.67

💡 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–	1.51	2.96	2.11	66	0.810	470	–	–
Hunt & Reffert	2024	1.51	2.92	2.11	55	–	470⁽¹⁾	–	–
Cavallo et al.	2024	1.79	3.02	–	78	0.810	–	–	–
Hunt & Reffert	2023	1.51	2.92	2.11	55	–	–	–	–
He et al.	2023	1.51	3.00	–	447	–	–	–	–

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

Visualization

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