CWNU 4101

0.00 UTI

0.0

C_N

0.3

C_dens

0.62

C_C3

0.0

C_lit

0.0

C_dup

C3 classification AC

Number of members (P>50%) 21

Radius (P>50% members) 10.7 [arcmin]

C_N 0.0 Sparse
C_dens 0.3 Loose
C_C3 0.62 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.0 Very likely duplicate

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

Overview

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CWNU 4101 is a sparse, 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 very 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 4101 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	–	114.784	-17.099	0.832	-2.848	1.045	28.902
He et al.	2023	114.896	-17.256	0.808	-2.83	1.049	32.16

💡 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	1.17	0.20	–	200	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Theia 3260	100.0	114.77	-17.1	0.84	-2.83	1.05	28.9	0.27

💡 Note: The % column shows the percentage of members that CWNU 4101 shares with each listed object.

Visualization

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