CWNU 2376

0.21 UTI

0.0

C_N

0.66

C_dens

0.38

C_C3

0.0

C_lit

1.0

C_dup

N_m (P>50%) 24

Core radius and density 0.8 [pc], 3.3 [pc^-2]

C3 classification CB

C_N 0.0 Sparse
C_dens 0.66 Moderately dense
C_C3 0.38 Low 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 2376 is a sparse, moderately dense object of low C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a very young cluster (see Parameters). It was recently reported in the literature.

⚠️ Warning: the low UTI value and no obvious signs of duplication (C_dup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Distant Moderate extinction Very young

Data

🔍 Search references for CWNU 2376 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–	123.388	-31.554	0.228	-3.105	4.812	–
He et al.	2023	123.388	-31.552	0.229	-3.105	4.812	–

💡 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–	3.89	1.7	–	16	–	–	–	–
He et al.	2023	3.89	1.70	–	16	–	–	–	–

Visualization

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