CWNU 3882

0.45 UTI

0.55

C_N

0.69

C_dens

1.0

C_C3

0.0

C_lit

1.0

C_dup

N₅₀ (P>50% members) 59

Stellar density (N₅₀/rad) 3.5 [N/pc²]

C3 classification AA

C_N 0.55 Moderately populated
C_dens 0.69 Moderately dense
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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CWNU 3882 is a moderately populated, moderately dense object of very high C3 quality. Its parallax locates it at a large^* distance, below 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.

(*): The parallax distance estimate (~8.87 kpc) differs significantly from the median photometric distance (~6.76 kpc).

Very distant Very high extinction Very young

Data

🔍 Search references for CWNU 3882 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–	166.087	-61.757	0.113	-5.871	2.282	32.991
He et al.	2023	166.085	-61.755	0.132	-5.869	2.282	38.22

💡 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–	6.76	6.35	–	10	–	–	–	–
He et al.	2023	6.76	6.35	–	10	–	–	–	–

Visualization

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