CWNU 1454

0.30 UTI

0.27

C_N

0.21

C_dens

0.5

C_C3

0.25

C_lit

1.0

C_dup

N₅₀ (P>50% members) 27

Stellar density (N₅₀/rad) 1.0 [N/pc²]

C3 classification BB

C_N 0.27 Poorly populated
C_dens 0.21 Very loose
C_C3 0.5 Intermediate 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 1454 is a poorly populated, very loose object of intermediate 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 (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 1454 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–	355.309	60.638	0.435	-2.958	-2.14	35.784
Hunt & Reffert	2024	355.27	60.645	0.443	-3.005	-2.102	35.706
Cavallo et al.	2024	355.191	60.657	0.446	–	–	–
Hunt & Reffert	2023	355.27	60.645	0.443	-3.005	-2.102	35.706
He et al.	2023	355.33	60.65	0.439	-2.961	-2.123	-46.84

💡 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–	2.19	3.41	2.29	44	0.890	254	–	–
Hunt & Reffert	2024	–	–	–	–	–	254⁽¹⁾	–	–
Cavallo et al.	2024	2.48	2.96	–	44	0.890	–	–	–
Hunt & Reffert	2023	2.13	3.41	2.29	37	–	–	–	–
He et al.	2023	2.19	3.45	–	100	–	–	–	–

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

Visualization

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