CWNU 4041

0.05 UTI

0.0

C_N

0.03

C_dens

0.38

C_C3

0.0

C_lit

0.64

C_dup

C3 classification CB

Number of members (P>50%) 14

Radius (P>50% members) 6.4 [arcmin]

C_N 0.0 Sparse
C_dens 0.03 Very loose
C_C3 0.38 Low quality
C_lit 0.0 Rarely studied
C_dup 0.64 Likely unique

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

Overview

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CWNU 4041 is a sparse, very loose object of low C3 quality. Its parallax locates it at a large^* distance, near the mid-plane, affected by high extinction. It is catalogued as a young cluster (see Parameters). It was recently reported in the literature.

(*): The parallax distance estimate (~5.03 kpc) differs significantly from the median photometric distance (~3.80 kpc).

Note: This is likely a unique object, which shares a moderate percentage of members with at least one previously reported entry. See table with shared members information.

Distant High extinction Young

Data

🔍 Search references for CWNU 4041 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	–	126.628	-38.874	0.199	-2.766	3.392	54.368
He et al.	2023	126.5	-38.881	0.202	-2.768	3.377	56.13

💡 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	3.80	3.50	–	40	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 2066	36.0	126.76	-38.89	0.18	-2.76	3.38	-66.47	0.13

💡 Note: The % column shows the percentage of members that CWNU 4041 shares with each listed object.

Visualization

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