CWNU 1095

0.31 UTI

0.25

C_N

0.28

C_dens

0.5

C_C3

0.25

C_lit

1.0

C_dup

N₅₀ (P>50% members) 25

Stellar density (N₅₀/rad) 1.4 [N/pc²]

C3 classification BB

C_N 0.25 Poorly populated
C_dens 0.28 Loose
C_C3 0.5 Intermediate quality
C_lit 0.25 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 1095 is a poorly populated, loose object of intermediate C3 quality. Its parallax locates it at a very close distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is poorly studied in the literature.

Very close Low extinction Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as a moving group.

Data

🔍 Search references for CWNU 1095 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–	171.594	64.047	4.077	11.651	2.105	-9.634
Zhang et al.	2024	171.352	63.84	–	–	–	–
Cavallo et al.	2024	166.088	60.191	4.01	–	–	–
Hunt & Reffert	2023	171.352	63.84	3.997	10.397	2.076	-8.226
He et al.	2022	172.561	63.868	4.132	11.838	1.765	–

💡 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–	0.25	0.35	0.5	257	0.251	–	–	–
Zhang et al.	2024	–	–	–	–	0.101⁽¹⁾	–	–	–
Cavallo et al.	2024	0.26	0.35	–	257	0.400	–	–	–
Hunt & Reffert	2023	0.24	0.11	0.50	254	–	–	–	–
He et al.	2022	–	0.45	–	398	–	–	–	–

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

Visualization

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