CWNU 3822

0.02 UTI

0.0

C_N

1.0

C_dens

0.5

C_C3

0.0

C_lit

0.08

C_dup

N₅₀ (P>50% members) 23

Stellar density (N₅₀/rad) 10.2 [N/pc²]

C3 classification BB

C_N 0.0 Sparse
C_dens 1.0 Very dense
C_C3 0.5 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.08 Very likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19

MOCA 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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CWNU 3822 is a sparse, very dense object of intermediate C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by very high extinction. It is catalogued as a very young cluster (see Parameters). It was recently reported in the literature.

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

Very distant Very high extinction Very young

Data

🔍 Search references for CWNU 3822 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	99999–	294.284	20.493	0.213	-2.643	-5.802	180.824
He et al.	2023	294.276	20.492	0.205	-2.628	-5.805	180.82

💡 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]	B_frac	BSS
UCC	99999–	5.75	5.5	–	5	–	–	–	–
He et al.	2023	5.75	5.50	–	5	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 458	92.0	294.28	20.49	0.2	-2.66	-5.79	180.82	0.35

💡 Note: The % column shows the percentage of members that CWNU 3822 shares with each listed object.

Visualization

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