CWNU 288

0.08 UTI

0.0

C_N

0.66

C_dens

0.75

C_C3

0.0

C_lit

0.28

C_dup

C3 classification AB

Number of members (P>50%) 22

Radius (P>50% members) 4.2 [arcmin]

C_N 0.0 Sparse
C_dens 0.66 Moderately dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.28 Possibly duplicate

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

Overview

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CWNU 288 is a sparse, moderately dense object of high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is rarely studied 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.

Relatively close Moderate extinction Near-solar metallicity Intermediate age

Data

🔍 Search references for CWNU 288 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	–	98.449	-1.716	0.474	-0.068	-0.854	–
He et al.	2022	98.45	-1.742	0.48	0.05	-0.84	42.1

💡 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	2.14	2.40	–	126	0.169	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
OC 0354	72.0	98.42	-1.72	0.47	-0.09	-0.88	24.19	0.36

💡 Note: The % column shows the percentage of members that CWNU 288 shares with each listed object.

Visualization

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