CWNU 2293

0.25 UTI

0.26

C_N

0.16

C_dens

0.25

C_C3

0.3

C_lit

1.0

C_dup

N₅₀ (P>50% members) 26

Stellar density (N₅₀/rad) 0.8 [N/pc²]

C3 classification DB

C_N 0.26 Poorly populated
C_dens 0.16 Very loose
C_C3 0.25 Low 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 2293 is a poorly populated, very loose object of low C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It was recently reported in the literature.

Relatively close Moderate extinction Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Gold sample.

Data

🔍 Search references for CWNU 2293 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–	103.922	-3.872	0.351	-1.111	2.37	60.159
Zhang et al.	2024	103.938	-3.769	–	–	–	–
Hunt & Reffert	2024	103.938	-3.769	0.341	-1.086	2.341	64.47
Cavallo et al.	2024	103.82	-3.798	0.341	–	–	–
Hunt & Reffert	2023	103.938	-3.769	0.341	-1.086	2.341	64.47
He et al.	2023	103.884	-3.808	0.369	-1.108	2.358	59.86

💡 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–	2.6	1.61	2.12	273	0.147	294	–	–
Zhang et al.	2024	–	–	–	–	-0.255⁽¹⁾	–	–	–
Hunt & Reffert	2024	–	–	–	–	–	294⁽¹⁾	–	–
Cavallo et al.	2024	2.65	1.61	–	275	0.550	–	–	–
Hunt & Reffert	2023	2.60	1.52	2.12	273	–	–	–	–
He et al.	2023	2.57	2.05	–	224	–	–	–	–

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

Visualization

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