CWNU 4369

0.09 UTI

0.31

C_N

0.05

C_dens

0.75

C_C3

0.0

C_lit

0.42

C_dup

C3 classification AB

Number of members (P>50%) 31

Radius (P>50% members) 4.3 [arcmin]

C_N 0.31 Poorly populated
C_dens 0.05 Very loose
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.42 Possibly duplicate

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

Overview

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CWNU 4369 is a poorly populated, very loose object of 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.

⚠️ 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.

Extremely distant Very high extinction Very young

Data

🔍 Search references for CWNU 4369 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	–	179.011	-63.315	0.114	-5.799	1.045	-44.869
He et al.	2023	179.04	-63.316	0.142	-5.78	1.028	–

💡 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	10.00	6.00	–	5	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
VVV 009	58.1	179.02	-63.32	0.09	-5.89	1.08	135.0	0.27

💡 Note: The % column shows the percentage of members that CWNU 4369 shares with each listed object.

Visualization

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