CWNU 1966

0.60 UTI

0.5

C_N

1.0

C_dens

0.75

C_C3

0.38

C_lit

1.0

C_dup

C3 classification BA

Number of members (P>50%) 51

Radius (P>50% members) 1.5 [arcmin]

C_N 0.5 Moderately populated
C_dens 1.0 Very dense
C_C3 0.75 High quality
C_lit 0.38 Poorly studied
C_dup 1.0 Unique

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

Overview

ℹ️

CWNU 1966 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It was recently reported in the literature.

Distant Moderate extinction Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Gold sample.

Data

🔍 Search references for CWNU 1966 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	104.18	0.471	0.222	-0.891	-0.029	33.755
Hu & Soubiran	2025	104.157	0.496	–	–	–	–
Zhang et al.	2024	104.18	0.472	–	–	–	–
Hunt & Reffert	2024	104.18	0.472	0.234	-0.858	-0.055	33.755
Cavallo et al.	2024	104.157	0.496	0.232	–	–	–
Hunt & Reffert	2023	104.18	0.472	0.234	-0.858	-0.055	33.755
He et al.	2023	104.18	0.48	0.258	-0.903	-0.031	64.41

💡 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]	Bfr	BSS
Hu & Soubiran	2025	–	–	–	–	-0.340*	–	–	–
Zhang et al.	2024	–	–	–	–	-0.067*	–	–	–
Hunt & Reffert	2024	–	–	–	–	–	652*	–	–
Cavallo et al.	2024	3.25	1.41	–	851	0.000	–	–	–
Hunt & Reffert	2023	3.66	1.41	2.53	288	–	–	–	–
He et al.	2023	3.63	1.55	–	794	–	–	–	–

(*): Indicates that this parameter is assigned more than one value in the corresponding reference.

Visualization

ℹ️

1 2