CWNU 3373

0.05 UTI

0.51

C_N

0.39

C_dens

0.75

C_C3

0.0

C_lit

0.15

C_dup

C3 classification BA

Number of members (P>50%) 52

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

C_N 0.51 Moderately populated
C_dens 0.39 Loose
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.15 Likely duplicate

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

Overview

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CWNU 3373 is a moderately populated, loose object of high C3 quality. Its parallax locates it at a large distance, above the mid-plane, affected by very high extinction. It is catalogued as a young 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.

Very distant Very high extinction Young

Data

🔍 Search references for CWNU 3373 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	–	289.562	14.455	0.17	-1.492	-4.004	31.125
He et al.	2023	289.566	14.456	0.186	-1.496	-4.01	31.13

💡 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	6.31	5.20	–	63	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 408	84.6	289.56	14.46	0.17	-1.49	-3.99	31.13	0.33

💡 Note: The % column shows the percentage of members that CWNU 3373 shares with each listed object.

Visualization

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