CWNU 95

0.24 UTI

0.47

C_N

1.0

C_dens

0.75

C_C3

0.35

C_lit

0.4

C_dup

N₅₀ (P>50% members) 47

Stellar density (N₅₀/rad) 37.5 [N/pc²]

C3 classification AB

C_N 0.47 Poorly populated
C_dens 1.0 Very dense
C_C3 0.75 High quality
C_lit 0.35 Poorly studied
C_dup 0.4 Possibly duplicate

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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CWNU 95 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by moderate extinction. It is catalogued as a very metal-poor, very young cluster, but with a large variance across recent sources for the absorption and metallicity parameters (see Parameters). It is poorly 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 Very metal-poor Very young

Liu et al. (2025)
Classified as tidal capture (resonant trapping binary) 55 along with NGC_5749.

Palma et al. (2025)
Classified as optical pair P379, along with NGC_5749.

Cavallo et al. (2024)
Gold sample.

Data

🔍 Search references for CWNU 95 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–	223.292	-54.102	0.909	-2.796	-2.301	-17.204
Hunt & Reffert	2024	223.297	-54.112	0.904	-2.858	-2.311	-15.491
Cavallo et al.	2024	222.843	-54.217	0.913	–	–	–
Hunt & Reffert	2023	223.297	-54.112	0.904	-2.858	-2.311	-15.491
He et al.	2022	223.304	-54.118	0.901	-2.806	-2.3	–
He et al.	2022	223.296	-54.111	0.91	-2.8	-2.3	–

💡 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–	1.055	1.08	1.41	16	-1.039	184	–	–
Liu et al.	2025	1.51	0.35	–	25	–	–	–	–
Hunt & Reffert	2024	–	–	–	–	–	184⁽¹⁾	–	–
Cavallo et al.	2024	1.08	1.15	–	12	-0.050	–	–	–
Hunt & Reffert	2023	1.03	1.08	1.41	23	–	–	–	–
He et al.	2022	–	1.05	–	11	–	–	–	–
He et al.	2022	0.85	1.38	–	16	-2.028	–	–	–

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

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWWDL 14468	85.1	223.29	-54.1	0.91	-2.81	-2.31	-17.2	0.0
OC 0623	59.6	223.29	-54.1	0.91	-2.83	-2.3	-17.2	0.41

💡 Note: The % column shows the percentage of members that CWNU 95 shares with each listed object.

Visualization

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