CWNU 2384

0.16 UTI

0.49

C_N

1.0

C_dens

0.75

C_C3

0.0

C_lit

0.37

C_dup

C3 classification AB

Number of members (P>50%) 49

Radius (P>50% members) 2.0 [arcmin]

C_N 0.49 Poorly populated
C_dens 1.0 Very dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.37 Possibly duplicate

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

Overview

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CWNU 2384 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by very high extinction. It is catalogued as an intermediate-age cluster (see Parameters). It was recently reported in the literature.

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

Relatively close Very high extinction Intermediate age

Data

🔍 Search references for CWNU 2384 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	–	194.451	-63.269	0.285	-6.717	-0.049	-22.612
He et al.	2023	194.447	-63.269	0.288	-6.721	-0.05	-22.61

💡 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	2.88	5.10	–	251	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Teutsch 109	63.3	194.46	-63.27	0.27	-6.71	-0.05	-22.61	0.54

💡 Note: The % column shows the percentage of members that CWNU 2384 shares with each listed object.

Visualization

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