CWNU 1733

0.38 UTI

0.3

C_N

0.6

C_dens

0.5

C_C3

0.25

C_lit

1.0

C_dup

N₅₀ (P>50% members) 30

Radius (P>50% members) 5.9 [arcmin]

C3 classification BB

C_N 0.3 Poorly populated
C_dens 0.6 Moderately dense
C_C3 0.5 Intermediate quality
C_lit 0.25 Poorly studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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CWNU 1733 is a poorly populated, moderately dense object of intermediate C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.

Relatively close Low extinction Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Gold sample.

Data

🔍 Search references for CWNU 1733 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–	114.216	-26.275	0.543	-2.845	2.991	46.785
Hunt & Reffert	2024	114.24	-26.321	0.536	-2.828	2.975	35.887
Cavallo et al.	2024	114.255	-26.3	0.538	–	–	–
Hunt & Reffert	2023	114.24	-26.321	0.536	-2.828	2.975	35.887
He et al.	2023	114.231	-26.302	0.544	-2.825	2.993	–

💡 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–	1.74	0.61	0.63	200	-0.280	81	–	–
Hunt & Reffert	2024	–	–	–	–	–	81⁽¹⁾	–	–
Cavallo et al.	2024	1.61	0.61	–	339	-0.280	–	–	–
Hunt & Reffert	2023	1.74	0.35	0.63	200	–	–	–	–
He et al.	2023	1.74	0.65	–	112	–	–	–	–

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

Visualization

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