CWNU 3573

0.11 UTI

0.46

C_N

0.38

C_dens

0.38

C_C3

0.0

C_lit

0.46

C_dup

C3 classification BC

Number of members (P>50%) 46

Radius (P>50% members) 2.9 [arcmin]

C_N 0.46 Poorly populated
C_dens 0.38 Loose
C_C3 0.38 Low quality
C_lit 0.0 Rarely studied
C_dup 0.46 Possibly duplicate

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

Overview

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CWNU 3573 is a poorly populated, loose object of low C3 quality. Its parallax locates it at a large distance, above the mid-plane, affected by moderate extinction. It is catalogued as a very 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.

Very distant Moderate extinction Very young

Data

🔍 Search references for CWNU 3573 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	–	82.67	38.628	0.172	0.056	-0.862	-39.378
He et al.	2023	82.652	38.625	0.156	0.054	-0.864	-31.45

💡 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	3.00	–	10	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 1328	54.3	82.69	38.61	0.18	0.06	-0.86	-31.45	0.13

💡 Note: The % column shows the percentage of members that CWNU 3573 shares with each listed object.

Visualization

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