CWNU 3399

0.06 UTI

0.0

C_N

1.0

C_dens

0.25

C_C3

0.0

C_lit

0.24

C_dup

C3 classification DB

Number of members (P>50%) 22

Radius (P>50% members) 1.5 [arcmin]

C_N 0.0 Sparse
C_dens 1.0 Very dense
C_C3 0.25 Low quality
C_lit 0.0 Rarely studied
C_dup 0.24 Likely duplicate

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

Overview

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CWNU 3399 is a sparse, very dense object of low C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by high 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.

Distant High extinction Intermediate age

Data

🔍 Search references for CWNU 3399 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	–	331.268	56.336	0.22	-3.648	-2.897	-84.034
He et al.	2023	331.272	56.333	0.226	-3.642	-2.899	-69.73

💡 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	4.17	3.85	–	158	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 787	76.0	331.28	56.33	0.22	-3.67	-2.89	-84.03	0.28

💡 Note: The % column shows the percentage of members that CWNU 3399 shares with each listed object.

Visualization

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