CWNU 419

0.03 UTI

0.33

C_N

0.11

C_dens

0.75

C_C3

0.0

C_lit

0.12

C_dup

N_m (P>50%) 33

Core radius and density 1.8 [pc], 0.6 [pc^-2]

C3 classification AB

C_N 0.33 Poorly populated
C_dens 0.11 Very loose
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.12 Likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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CWNU 419 is a poorly populated, very loose object of high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is rarely studied in the literature.

⚠️ Warning: This is likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

Relatively close Moderate extinction Near-solar metallicity Intermediate age

Data

🔍 Search references for CWNU 419 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–	346.896	58.918	0.663	-1.806	-1.498	-17.615
He et al.	2022	346.857	58.907	0.66	-1.81	-1.5	–

💡 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–	1.82	1.27	–	251	0.398	–	–	–
He et al.	2022	1.82	1.27	–	251	0.398	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Theia 2902	100.0	346.86	58.9	0.65	-1.81	-1.5	-17.61	0.14
UBC 1574	87.9	346.9	58.91	0.66	-1.8	-1.5	-17.61	0.25
CWWDL 14151	78.8	346.94	58.95	0.66	-1.8	-1.5	-17.61	0.02

💡 Note: The % column shows the percentage of members that CWNU 419 shares with each listed object.

Visualization

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