CWNU 4050

0.03 UTI

0.3

C_N

0.08

C_dens

0.62

C_C3

0.0

C_lit

0.17

C_dup

C3 classification AC

Number of members (P>50%) 30

Radius (P>50% members) 5.1 [arcmin]

C_N 0.3 Poorly populated
C_dens 0.08 Very loose
C_C3 0.62 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.17 Likely duplicate

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

Overview

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CWNU 4050 is a poorly populated, very loose object of intermediate C3 quality. Its parallax locates it at a large distance, above the mid-plane, affected by moderate extinction. It is catalogued as a 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.

Very distant Moderate extinction Young

Data

🔍 Search references for CWNU 4050 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	–	91.4	23.515	0.171	0.25	-0.425	–
He et al.	2023	91.383	23.504	0.182	0.252	-0.446	18.18

💡 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	5.01	2.10	–	40	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 1480	83.3	91.41	23.52	0.17	0.27	-0.42	–	0.3

💡 Note: The % column shows the percentage of members that CWNU 4050 shares with each listed object.

Visualization

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