CWNU 1443

0.25 UTI

0.25

C_N

0.14

C_dens

0.38

C_C3

0.25

C_lit

1.0

C_dup

N₅₀ (P>50% members) 25

Stellar density (N₅₀/rad) 0.7 [N/pc²]

C3 classification BC

C_N 0.25 Poorly populated
C_dens 0.14 Very loose
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

ℹ️

CWNU 1443 is a poorly populated, very loose 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, but with a large variance across recent sources for the absorption and age parameters (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 1443 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	99999–	114.113	-26.011	0.253	-1.883	2.842	–
Hunt & Reffert	2024	114.119	-26.063	0.231	-1.848	2.882	–
Cavallo et al.	2024	114.125	-26.033	0.237	–	–	–
Hunt & Reffert	2023	114.119	-26.063	0.231	-1.848	2.882	–
He et al.	2023	114.131	-26.048	0.277	-1.935	2.801	–

💡 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–	3.61	1.42	0.84	90	0.040	150	–	–
Hunt & Reffert	2024	–	–	–	–	–	150⁽¹⁾	–	–
Cavallo et al.	2024	3.15	1.52	–	95	0.040	–	–	–
Hunt & Reffert	2023	3.61	1.42	0.84	90	–	–	–	–
He et al.	2023	4.37	0.05	–	3	–	–	–	–

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

Visualization

ℹ️

1 2