CWNU 3141

0.09 UTI

0.79

C_N

1.0

C_dens

1.0

C_C3

0.0

C_lit

0.16

C_dup

C3 classification AA

Number of members (P>50%) 196

Radius (P>50% members) 2.3 [arcmin]

C_N 0.79 Rich
C_dens 1.0 Very dense
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 0.16 Likely duplicate

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

Overview

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CWNU 3141 is a rich, very dense object of very high C3 quality. Its parallax locates it at a large distance, below the mid-plane, affected by moderate 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.

Very distant Moderate extinction Intermediate age

Data

🔍 Search references for CWNU 3141 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	–	158.817	-60.691	0.139	-4.852	2.548	29.282
He et al.	2023	158.813	-60.691	0.138	-4.852	2.549	17.19

💡 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	5.62	2.00	–	794	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 2363	84.2	158.81	-60.69	0.14	-4.86	2.54	37.72	0.09
Teutsch 105	75.5	158.81	-60.69	0.14	-4.86	2.55	37.72	0.55

💡 Note: The % column shows the percentage of members that CWNU 3141 shares with each listed object.

Visualization

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