CWNU 3300

0.29 UTI

0.33

C_N

0.14

C_dens

1.0

C_C3

0.0

C_lit

1.0

C_dup

N_m (P>50%) 33

Core radius and density 2.5 [pc], 0.7 [pc^-2]

C3 classification AA

C_N 0.33 Poorly populated
C_dens 0.14 Very loose
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

MOCA 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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CWNU 3300 is a poorly populated, very loose object of very high C3 quality. Its parallax locates it at a very large distance, well below the mid-plane, affected by low extinction. It is catalogued as an intermediate-age cluster (see Parameters). It was recently reported in the literature.

Very distant Low extinction Intermediate age

Data

🔍 Search references for CWNU 3300 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	99999–	107.145	-23.128	0.093	-0.625	1.538	–
He et al.	2023	107.145	-23.13	0.087	-0.631	1.54	–

💡 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]	B_frac	BSS
UCC	99999–	8.32	0.2	–	794	–	–	–	–
He et al.	2023	8.32	0.20	–	794	–	–	–	–

Visualization

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