CWNU 28

0.00 UTI

0.31

C_N

0.56

C_dens

0.75

C_C3

0.0

C_lit

0.0

C_dup

N_m (P>50%) 31

Core radius and density 1.2 [pc], 2.8 [pc^-2]

C3 classification BA

C_N 0.31 Poorly populated
C_dens 0.56 Moderately dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.0 Very likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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CWNU 28 is a poorly populated, moderately dense object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, old cluster (see Parameters). It is rarely studied 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.

Relatively close Moderate extinction Near-solar metallicity Old

Data

🔍 Search references for CWNU 28 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–	280.39	-6.006	0.362	-1.513	-4.082	-10.13
He et al.	2022	280.388	-6.007	0.35	-1.53	-4.08	-12.9

💡 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–	2.19	1.9	–	1000	0.420	–	–	–
He et al.	2022	2.19	1.90	–	1000	0.420	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 1037	100.0	280.39	-6.0	0.35	-1.51	-4.08	-10.25	0.44

💡 Note: The % column shows the percentage of members that CWNU 28 shares with each listed object.

Visualization

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