CWNU 1479

0.44 UTI

0.45

C_N

1.0

C_dens

0.25

C_C3

0.25

C_lit

1.0

C_dup

N₅₀ (P>50% members) 45

Stellar density (N₅₀/rad) 5.6 [N/pc²]

C3 classification CC

C_N 0.45 Poorly populated
C_dens 1.0 Very dense
C_C3 0.25 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 1479 is a poorly populated, very dense object of low C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high 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 High extinction Metal-rich Young

Cavallo et al. (2024)
Gold sample.

Data

🔍 Search references for CWNU 1479 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–	61.432	51.813	0.442	0.182	-2.211	–
Hunt & Reffert	2024	61.449	51.8	0.432	0.201	-2.198	–
Cavallo et al.	2024	61.439	51.796	0.434	–	–	–
Hunt & Reffert	2023	61.449	51.8	0.432	0.201	-2.198	–
He et al.	2023	61.456	51.791	0.447	0.158	-2.226	–

💡 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–	2.11	3.04	1.8	79	0.510	389	–	–
Hunt & Reffert	2024	–	–	–	–	–	389⁽¹⁾	–	–
Cavallo et al.	2024	2.11	3.04	–	398	0.510	–	–	–
Hunt & Reffert	2023	2.15	3.33	1.80	79	–	–	–	–
He et al.	2023	2.04	1.25	–	3	–	–	–	–

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

Visualization

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