CWNU 415

0.02 UTI

0.0

C_N

0.08

C_dens

0.25

C_C3

0.0

C_lit

0.32

C_dup

N_m (P>50%) 23

Core radius and density 3.4 [pc], 0.4 [pc^-2]

C3 classification DB

C_N 0.0 Sparse
C_dens 0.08 Very loose
C_C3 0.25 Low quality
C_lit 0.0 Rarely studied
C_dup 0.32 Possibly duplicate

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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CWNU 415 is a sparse, very loose object of low 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, young cluster (see Parameters). It is rarely 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, and a moderate percentage with at least one entry reported in the same catalogue. See table with shared members information.

Relatively close Moderate extinction Near-solar metallicity Young

Data

🔍 Search references for CWNU 415 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–	347.861	57.411	0.91	0.239	-1.378	-23.498
He et al.	2022	347.644	57.342	0.91	0.21	-1.38	-25.8

💡 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–	1.1	1.77	–	50	0.350	–	–	–
He et al.	2022	1.10	1.77	–	50	0.350	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWWDL 14366	92.0	348.22	57.48	0.92	0.24	-1.34	-29.86	0.13
LISC 3420	68.0	348.1	57.47	0.91	0.26	-1.37	-31.89	0.23
Theia 2526	64.0	348.12	57.48	0.91	0.27	-1.37	-31.89	0.0
CWNU 83	44.0	347.51	57.0	0.91	0.19	-1.4	-19.28	0.04

💡 Note: The % column shows the percentage of members that CWNU 415 shares with each listed object.

Visualization

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