CWNU 3066

0.28 UTI

0.58

C_N

1.0

C_dens

0.62

C_C3

0.0

C_lit

0.63

C_dup

C3 classification AC

Number of members (P>50%) 67

Radius (P>50% members) 1.4 [arcmin]

C_N 0.58 Moderately populated
C_dens 1.0 Very dense
C_C3 0.62 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.63 Likely unique

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

Overview

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CWNU 3066 is a moderately populated, very dense object of intermediate C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as an old cluster (see Parameters). It was recently reported in the literature.

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.

Very distant High extinction Old

Data

🔍 Search references for CWNU 3066 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	–	185.973	-62.752	0.214	-8.459	1.37	-30.74
He et al.	2023	185.973	-62.752	0.202	-8.47	1.359	-30.74

💡 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	5.50	3.50	–	3981	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 2512	37.3	185.97	-62.75	0.19	-8.45	1.38	-30.74	0.43

💡 Note: The % column shows the percentage of members that CWNU 3066 shares with each listed object.

Visualization

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