CWNU 2864

0.25 UTI

0.0

C_N

0.52

C_dens

0.75

C_C3

0.0

C_lit

1.0

C_dup

N₅₀ (P>50% members) 17

Stellar density (N₅₀/rad) 2.6 [N/pc²]

C3 classification AB

C_N 0.0 Sparse
C_dens 0.52 Moderately dense
C_C3 0.75 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 2864 is a sparse, moderately dense object of high C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by high extinction. It is catalogued as a very young cluster (see Parameters). It was recently reported in the literature.

Relatively close High extinction Very young

Data

🔍 Search references for CWNU 2864 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–	279.401	-11.428	0.521	-0.992	-3.486	-2.502
He et al.	2023	279.427	-11.425	0.54	-0.993	-3.491	–

💡 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–	1.82	3.2	–	4	–	–	–	–
He et al.	2023	1.82	3.20	–	4	–	–	–	–

Visualization

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