CWNU 3412

0.10 UTI

0.55

C_N

1.0

C_dens

0.38

C_C3

0.0

C_lit

0.25

C_dup

C3 classification CB

Number of members (P>50%) 60

Radius (P>50% members) 2.0 [arcmin]

C_N 0.55 Moderately populated
C_dens 1.0 Very dense
C_C3 0.38 Low quality
C_lit 0.0 Rarely studied
C_dup 0.25 Possibly duplicate

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

Overview

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CWNU 3412 is a moderately populated, very dense object of low C3 quality. Its parallax locates it at a large distance, above the mid-plane, affected by very high extinction. It is catalogued as an intermediate-age cluster (see Parameters). It was recently reported in the literature.

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

Distant Very high extinction Intermediate age

Data

🔍 Search references for CWNU 3412 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	–	290.487	19.259	0.184	-1.302	-4.695	0.757
He et al.	2023	290.487	19.262	0.184	-1.297	-4.676	30.15

💡 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	4.57	5.15	–	794	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 438	75.0	290.49	19.25	0.18	-1.29	-4.68	0.76	0.36

💡 Note: The % column shows the percentage of members that CWNU 3412 shares with each listed object.

Visualization

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