CWNU 3510

0.12 UTI

0.43

C_N

0.18

C_dens

0.38

C_C3

0.0

C_lit

0.6

C_dup

N_m (P>50%) 43

Core radius and density 2.7 [pc], 0.9 [pc^-2]

C3 classification BC

C_N 0.43 Poorly populated
C_dens 0.18 Very loose
C_C3 0.38 Low quality
C_lit 0.0 Rarely studied
C_dup 0.6 Likely unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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CWNU 3510 is a poorly populated, very loose object of low C3 quality. Its parallax locates it at a large distance, above the mid-plane, affected by moderate extinction. It is catalogued as an old cluster (see Parameters). It was recently reported in the literature.

Note: This object contains blue stragglers according to at least one source.

Note: This is likely a unique object, which shares a moderate percentage of members with at least one previously reported entry. See table with shared members information.

Very distant Moderate extinction Old Contains BSS

Data

🔍 Search references for CWNU 3510 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–	149.845	-54.514	0.11	-4.498	2.581	64.66
Cui et al.	2025	149.842	-54.509	0.1	-4.5	2.58	–
He et al.	2023	149.844	-54.51	0.099	-4.497	2.582	84.64

💡 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–	7.24	2.75	–	2117	–	–	–	6
Cui et al.	2025	–	2.65	–	2239	–	–	–	6⁽¹⁾
He et al.	2023	7.24	2.85	–	1995	–	–	–	–

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

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
FSR 1518	39.5	149.84	-54.51	0.15	-4.54	2.58	57.33	0.19

💡 Note: The % column shows the percentage of members that CWNU 3510 shares with each listed object.

Visualization

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