CWNU 3283

0.07 UTI

0.0

C_N

0.18

C_dens

0.75

C_C3

0.0

C_lit

0.4

C_dup

C3 classification AB

Number of members (P>50%) 19

Radius (P>50% members) 3.0 [arcmin]

C_N 0.0 Sparse
C_dens 0.18 Very loose
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.4 Possibly duplicate

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

Overview

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CWNU 3283 is a sparse, very loose object of high C3 quality. Its parallax locates it at a large distance, near the mid-plane, affected by moderate extinction. It is catalogued as a young 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 Moderate extinction Young

Data

🔍 Search references for CWNU 3283 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	–	165.566	-60.002	0.191	-7.138	2.96	-32.64
He et al.	2023	165.538	-59.983	0.19	-7.154	2.956	-32.64

💡 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	4.27	2.15	–	32	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 2395	60.0	165.56	-60.0	0.19	-7.16	2.92	–	0.14

💡 Note: The % column shows the percentage of members that CWNU 3283 shares with each listed object.

Visualization

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