CWNU 2288

0.33 UTI

0.52

C_N

0.5

C_dens

0.5

C_C3

0.06

C_lit

1.0

C_dup

N_m (P>50%) 55

Core radius and density 1.3 [pc], 2.5 [pc^-2]

C3 classification BB

C_N 0.52 Moderately populated
C_dens 0.5 Moderately dense
C_C3 0.5 Intermediate quality
C_lit 0.06 Rarely studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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CWNU 2288 is a moderately populated, moderately dense object of intermediate C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It was recently reported in the literature.

Relatively close High extinction Near-solar metallicity Young

Cavallo et al. (2024)
Silver sample.

Hunt & Reffert (2024)
Classified as open cluster. CMD classes: 0.76 (50th percentile), false positive? (human-assigned).

Hunt & Reffert (2023)
Classified as open cluster. CMD classes: 0.76 (50th percentile), false positive? (human-assigned).

Data

🔍 Search references for CWNU 2288 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–	271.745	-18.242	0.512	0.438	-0.448	–
Hunt & Reffert	2024	271.729	-18.252	0.506	0.436	-0.468	–
Cavallo et al.	2024	271.734	-18.244	0.503	–	–	–
Hunt & Reffert	2023	271.729	-18.252	0.506	0.436	-0.468	–
He et al.	2023	271.749	-18.249	0.531	0.401	-0.456	–

💡 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–	1.81	3.76	2.38	88	0.050	329	–	–
Hunt & Reffert	2024	1.88	3.76	2.38	63	–	329⁽¹⁾	–	–
Cavallo et al.	2024	1.68	3.56	–	209	0.050	–	–	–
Hunt & Reffert	2023	1.88	3.76	2.38	63	–	–	–	–
He et al.	2023	1.74	4.20	–	112	–	–	–	–

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Visualization

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