CWNU 2341

0.03 UTI

0.0

C_N

0.59

C_dens

0.25

C_C3

0.0

C_lit

0.16

C_dup

C3 classification DB

Number of members (P>50%) 16

Radius (P>50% members) 1.4 [arcmin]

C_N 0.0 Sparse
C_dens 0.59 Moderately dense
C_C3 0.25 Low quality
C_lit 0.0 Rarely studied
C_dup 0.16 Likely duplicate

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

Overview

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CWNU 2341 is a sparse, moderately dense object of low C3 quality. Its parallax locates it at a large^* distance, below the mid-plane, affected by moderate extinction. It is catalogued as an intermediate-age cluster (see Parameters). It was recently reported in the literature.

⚠️ Warning: This is likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

(*): The parallax distance estimate (~5.72 kpc) differs significantly from the median photometric distance (~4.07 kpc).

Distant Moderate extinction Intermediate age

Data

🔍 Search references for CWNU 2341 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	–	97.081	2.953	0.175	0.017	0.445	46.68
He et al.	2023	97.016	3.062	0.207	0.113	0.498	61.82

💡 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
He et al.	2023	4.07	1.80	–	631	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
FSR 1033	84.0	97.07	2.95	0.18	-0.07	0.38	48.38	0.58

💡 Note: The % column shows the percentage of members that CWNU 2341 shares with each listed object.

Visualization

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