CWNU 3541

0.02 UTI

0.25

C_N

0.18

C_dens

0.38

C_C3

0.0

C_lit

0.12

C_dup

C3 classification CB

Number of members (P>50%) 25

Radius (P>50% members) 7.0 [arcmin]

C_N 0.25 Poorly populated
C_dens 0.18 Very loose
C_C3 0.38 Low 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 3541 is a poorly populated, very loose object of low C3 quality. Its parallax locates it at a moderate distance, near 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 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 Moderate extinction Very young

Data

🔍 Search references for CWNU 3541 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	–	154.692	-57.291	0.391	-7.783	4.147	–
He et al.	2023	154.666	-57.293	0.399	-7.779	4.168	–

💡 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	2.69	2.10	–	6	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 2324	88.0	154.69	-57.27	0.39	-7.78	4.15	–	0.11

💡 Note: The % column shows the percentage of members that CWNU 3541 shares with each listed object.

Visualization

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