CWNU 3408

0.03 UTI

0.29

C_N

0.34

C_dens

1.0

C_C3

0.0

C_lit

0.1

C_dup

C3 classification AA

Number of members (P>50%) 29

Radius (P>50% members) 4.1 [arcmin]

C_N 0.29 Poorly populated
C_dens 0.34 Loose
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 0.1 Likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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CWNU 3408 is a poorly populated, loose object of very high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate extinction. It is catalogued as an intermediate-age cluster (see Parameters). It was recently reported 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 Intermediate age

Data

🔍 Search references for CWNU 3408 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	–	295.097	17.778	0.289	-1.979	-2.552	19.436
He et al.	2023	295.098	17.777	0.289	-1.97	-2.554	–

💡 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]	Bfr	BSS
He et al.	2023	2.95	2.80	–	251	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 444	89.7	295.1	17.78	0.29	-1.97	-2.55	19.44	0.27

💡 Note: The % column shows the percentage of members that CWNU 3408 shares with each listed object.

Visualization

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