CWNU 4411

0.05 UTI

0.29

C_N

0.92

C_dens

0.75

C_C3

0.0

C_lit

0.14

C_dup

C3 classification BA

Number of members (P>50%) 29

Radius (P>50% members) 2.8 [arcmin]

C_N 0.29 Poorly populated
C_dens 0.92 Very dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.14 Likely duplicate

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

Overview

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CWNU 4411 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 likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

Distant Very high extinction Intermediate age

Data

🔍 Search references for CWNU 4411 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	–	277.072	-11.441	0.324	-0.458	-2.208	19.649
He et al.	2023	277.065	-11.464	0.318	-0.458	-2.21	29.54

💡 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	3.98	5.65	–	158	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 215	86.2	277.07	-11.45	0.32	-0.46	-2.21	29.54	0.38

💡 Note: The % column shows the percentage of members that CWNU 4411 shares with each listed object.

Visualization

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