CWNU 528

0.31 UTI

0.25

C_N

0.54

C_dens

0.75

C_C3

0.0

C_lit

1.0

C_dup

C3 classification AB

Number of members (P>50%) 25

Radius (P>50% members) 25.2 [arcmin]

C_N 0.25 Poorly populated
C_dens 0.54 Moderately dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 1.0 Unique

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

Overview

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CWNU 528 is a poorly populated, moderately dense object of high C3 quality. Its parallax locates it at a very close distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It is rarely studied in the literature.

Very close Low extinction Near-solar metallicity Young

Data

🔍 Search references for CWNU 528 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	–	110.278	-36.52	2.412	-5.893	6.362	12.079
He et al.	2022	108.038	-34.192	2.433	-5.536	6.403	–
He et al.	2022	110.242	-36.554	2.37	-5.82	6.37	–

💡 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.	2022	–	0.45	–	32	–	–	–	–
He et al.	2022	0.36	0.12	–	50	0.370	–	–	–

Visualization

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