CWNU 2692

0.27 UTI

0.3

C_N

0.17

C_dens

0.75

C_C3

0.06

C_lit

1.0

C_dup

N_m (P>50%) 30

Core radius and density 1.4 [pc], 0.8 [pc^-2]

C3 classification AB

C_N 0.3 Poorly populated
C_dens 0.17 Very loose
C_C3 0.75 High quality
C_lit 0.06 Rarely studied
C_dup 1.0 Unique

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MOCA 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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CWNU 2692 is a poorly populated, very loose object of high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It was recently reported in the literature.

Relatively close Low extinction Near-solar metallicity Young

Palma et al. (2025)
Part of multiple system G59, along with CWNU_277, HSC_2552, NGC_4755, Ruprecht_105 and CWNU_2664.

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as open cluster. CMD class: 1.00 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 1.00 (50th percentile).

Data

🔍 Search references for CWNU 2692 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–	194.069	-60.432	0.451	-5.64	-0.326	-26.75
Hunt & Reffert	2024	194.08	-60.446	0.45	-5.644	-0.323	–
Cavallo et al.	2024	194.093	-60.449	0.451	–	–	–
Hunt & Reffert	2023	194.08	-60.446	0.45	-5.644	-0.323	–
He et al.	2023	194.061	-60.458	0.449	-5.644	-0.308	-33.43

💡 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–	2.06	0.87	0.28	94	0.320	158	–	–
Hunt & Reffert	2024	2.03	0.78	0.28	83	–	158⁽¹⁾	–	–
Cavallo et al.	2024	2.27	0.96	–	105	0.320	–	–	–
Hunt & Reffert	2023	2.03	0.78	0.28	83	–	–	–	–
He et al.	2023	2.09	1.30	–	112	–	–	–	–

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

Visualization

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