CWNU 3483

0.11 UTI

0.32

C_N

1.0

C_dens

0.38

C_C3

0.0

C_lit

0.31

C_dup

C3 classification BC

Number of members (P>50%) 32

Radius (P>50% members) 1.4 [arcmin]

C_N 0.32 Poorly populated
C_dens 1.0 Very dense
C_C3 0.38 Low quality
C_lit 0.0 Rarely studied
C_dup 0.31 Possibly duplicate

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

Overview

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CWNU 3483 is a poorly populated, very dense object of low C3 quality. Its parallax locates it at a large 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 possibly a duplicate object, which shares a significant percentage of members with at least one previously reported entry. See table with shared members information.

Very distant Moderate extinction Intermediate age

Data

🔍 Search references for CWNU 3483 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	–	82.606	27.098	0.178	0.307	-0.686	4.057
He et al.	2023	82.604	27.098	0.185	0.336	-0.692	7.5

💡 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]	Bfr	BSS
He et al.	2023	5.89	2.30	–	794	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Teutsch 90	68.8	82.61	27.1	0.22	0.33	-0.69	7.5	0.29

💡 Note: The % column shows the percentage of members that CWNU 3483 shares with each listed object.

Visualization

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