CWNU 2142

0.44 UTI

0.0

C_N

0.83

C_dens

0.75

C_C3

0.31

C_lit

1.0

C_dup

C3 classification AB

Number of members (P>50%) 20

Radius (P>50% members) 1.9 [arcmin]

C_N 0.0 Sparse
C_dens 0.83 Dense
C_C3 0.75 High quality
C_lit 0.31 Poorly studied
C_dup 1.0 Unique

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

Overview

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CWNU 2142 is a sparse, dense object of high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the age parameter (see Parameters). It was recently reported in the literature.

Distant Low extinction Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Gold sample.

Data

🔍 Search references for CWNU 2142 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	–	90.365	27.637	0.252	0.835	-0.119	–
Hu & Soubiran	2025	90.357	27.628	–	–	–	–
Hunt & Reffert	2024	90.36	27.633	0.245	0.835	-0.118	–
Cavallo et al.	2024	90.357	27.628	0.243	–	–	–
Hunt & Reffert	2023	90.36	27.633	0.245	0.835	-0.118	–
He et al.	2023	90.353	27.632	0.252	0.843	-0.119	–

💡 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	–	–	–	–	-0.250*	–	–	–
Hunt & Reffert	2024	–	–	–	–	–	141*	–	–
Cavallo et al.	2024	3.12	0.69	–	776	-0.020	–	–	–
Hunt & Reffert	2023	4.08	1.00	1.30	185	–	–	–	–
He et al.	2023	3.63	1.35	–	126	–	–	–	–

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

Visualization

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