CWNU 2352

0.54 UTI

0.31

C_N

1.0

C_dens

1.0

C_C3

0.25

C_lit

0.97

C_dup

C3 classification AA

Number of members (P>50%) 31

Radius (P>50% members) 2.1 [arcmin]

C_N 0.31 Poorly populated
C_dens 1.0 Very dense
C_C3 1.0 Very high quality
C_lit 0.25 Poorly studied
C_dup 0.97 Unique

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

Overview

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CWNU 2352 is a poorly populated, very dense object of very high 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, intermediate-age cluster (see Parameters). It was recently reported in the literature.

Note: This is a unique object, which shares a very small percentage of members with at least one previously reported entry. See table with shared members information.

Distant Moderate extinction Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Gold sample.

Data

🔍 Search references for CWNU 2352 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	–	35.375	57.994	0.287	-1.339	-0.418	–
Hunt & Reffert	2024	35.389	57.998	0.287	-1.337	-0.414	–
Cavallo et al.	2024	35.353	57.997	0.287	–	–	–
Hunt & Reffert	2023	35.389	57.998	0.287	-1.337	-0.414	–
He et al.	2023	35.346	58.011	0.296	-1.335	-0.39	-53.69

💡 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
Hunt & Reffert	2024	–	–	–	–	–	321*	–	–
Cavallo et al.	2024	3.58	2.43	–	66	0.040	–	–	–
Hunt & Reffert	2023	3.13	2.18	0.67	100	–	–	–	–
He et al.	2023	3.09	2.35	–	141	–	–	–	–

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

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
FoF 921	3.2	35.61	58.0	0.26	-1.04	-0.37	-37.7	0.03

💡 Note: The % column shows the percentage of members that CWNU 2352 shares with each listed object.

Visualization

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