CWNU 1088

0.42 UTI

0.25

C_N

0.52

C_dens

0.75

C_C3

0.3

C_lit

1.0

C_dup

N₅₀ (P>50% members) 25

Stellar density (N₅₀/rad) 2.6 [N/pc²]

C3 classification AB

C_N 0.25 Poorly populated
C_dens 0.52 Moderately dense
C_C3 0.75 High quality
C_lit 0.3 Poorly studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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CWNU 1088 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 moderate extinction. It is catalogued as a near-solar metallicity, very young cluster, but with a large variance across recent sources for the age parameter (see Parameters). It is poorly studied in the literature.

Close Moderate extinction Near-solar metallicity Very young

Cavallo et al. (2024)
Wood sample.

Data

🔍 Search references for CWNU 1088 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–	86.078	-1.433	2.218	1.621	-4.027	10.31
Zhang et al.	2024	85.906	-1.593	–	–	–	–
Hunt & Reffert	2024	85.906	-1.593	2.213	1.698	-4.061	17.033
Cavallo et al.	2024	86.548	-1.313	2.21	–	–	–
Hunt & Reffert	2023	85.906	-1.593	2.213	1.698	-4.061	17.033
He et al.	2022	86.076	-1.326	2.217	1.596	-4.034	–

💡 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–	0.525	2.97	2.38	8	0.037	72	–	–
Zhang et al.	2024	–	–	–	–	-0.075⁽¹⁾	–	–	–
Hunt & Reffert	2024	–	–	–	–	–	72⁽¹⁾	–	–
Cavallo et al.	2024	0.61	2.97	–	8	0.150	–	–	–
Hunt & Reffert	2023	0.44	2.52	2.38	30	–	–	–	–
He et al.	2022	–	4.10	–	3	–	–	–	–

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

Visualization

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