CWNU 1679

0.37 UTI

0.33

C_N

0.66

C_dens

0.38

C_C3

0.25

C_lit

1.0

C_dup

N₅₀ (P>50% members) 33

Stellar density (N₅₀/rad) 3.3 [N/pc²]

C3 classification CB

C_N 0.33 Poorly populated
C_dens 0.66 Moderately dense
C_C3 0.38 Low quality
C_lit 0.25 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 1679 is a poorly populated, moderately dense object of low C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It was recently reported in the literature.

Distant Moderate extinction Near-solar metallicity Young

Cavallo et al. (2024)
Gold sample.

Data

🔍 Search references for CWNU 1679 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–	119.023	-32.126	0.295	-2.943	2.663	–
Hunt & Reffert	2024	119.034	-32.155	0.29	-2.949	2.683	–
Cavallo et al.	2024	119.0	-32.106	0.293	–	–	–
Hunt & Reffert	2023	119.034	-32.155	0.29	-2.949	2.683	–
He et al.	2023	119.021	-32.134	0.32	-2.949	2.656	–

💡 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–	3.16	2.02	1.09	70	0.480	347	–	–
Hunt & Reffert	2024	–	–	–	–	–	347⁽¹⁾	–	–
Cavallo et al.	2024	3.08	1.91	–	115	0.480	–	–	–
Hunt & Reffert	2023	3.17	2.02	1.09	70	–	–	–	–
He et al.	2023	3.16	2.35	–	35	–	–	–	–

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

Visualization

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