CWNU 3571

0.02 UTI

0.0

C_N

0.16

C_dens

0.62

C_C3

0.0

C_lit

0.12

C_dup

C3 classification AC

Number of members (P>50%) 22

Radius (P>50% members) 13.4 [arcmin]

C_N 0.0 Sparse
C_dens 0.16 Very loose
C_C3 0.62 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.12 Likely duplicate

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

Overview

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CWNU 3571 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by low extinction. It is catalogued as an intermediate-age 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.

Relatively close Low extinction Intermediate age

Data

🔍 Search references for CWNU 3571 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	–	91.582	37.291	0.75	0.857	-4.432	-20.595
He et al.	2023	91.61	37.261	0.745	0.839	-4.436	-24.71

💡 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	1.41	0.95	–	398	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 1367	88.0	91.53	37.29	0.75	0.87	-4.43	-21.29	0.29

💡 Note: The % column shows the percentage of members that CWNU 3571 shares with each listed object.

Visualization

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