CWNU 4758

0.03 UTI

0.28

C_N

0.29

C_dens

0.5

C_C3

0.0

C_lit

0.14

C_dup

C3 classification BB

Number of members (P>50%) 28

Radius (P>50% members) 2.6 [arcmin]

C_N 0.28 Poorly populated
C_dens 0.29 Loose
C_C3 0.5 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.14 Likely duplicate

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

Overview

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CWNU 4758 is a poorly populated, 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 4758 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	–	127.452	-32.265	0.171	-2.137	2.542	90.112
He et al.	2023	127.449	-32.264	0.172	-2.128	2.549	83.47

💡 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	1.60	–	25	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 2027	85.7	127.45	-32.26	0.17	-2.13	2.55	96.75	0.26

💡 Note: The % column shows the percentage of members that CWNU 4758 shares with each listed object.

Visualization

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