CWNU 4060

0.05 UTI

0.26

C_N

0.73

C_dens

0.25

C_C3

0.0

C_lit

0.19

C_dup

C3 classification CC

Number of members (P>50%) 26

Radius (P>50% members) 9.0 [arcmin]

C_N 0.26 Poorly populated
C_dens 0.73 Moderately dense
C_C3 0.25 Low quality
C_lit 0.0 Rarely studied
C_dup 0.19 Likely duplicate

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

Overview

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CWNU 4060 is a poorly populated, moderately dense object of low C3 quality. Its parallax locates it at a relatively close 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.

Relatively close Moderate extinction Young

Data

🔍 Search references for CWNU 4060 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	–	48.718	61.18	0.979	1.956	-3.658	-8.786
He et al.	2023	48.722	61.18	0.991	1.945	-3.667	–

💡 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	1.05	1.60	–	32	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 1127	80.8	48.72	61.18	0.99	1.95	-3.67	-13.97	0.22

💡 Note: The % column shows the percentage of members that CWNU 4060 shares with each listed object.

Visualization

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