CWNU 1327

0.40 UTI

0.28

C_N

0.97

C_dens

0.75

C_C3

0.0

C_lit

1.0

C_dup

N₅₀ (P>50% members) 28

Stellar density (N₅₀/rad) 4.8 [N/pc²]

C3 classification AB

C_N 0.28 Poorly populated
C_dens 0.97 Very 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 1327 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as an intermediate-age cluster (see Parameters). It was recently reported in the literature.

Relatively close High extinction Intermediate age

Data

🔍 Search references for CWNU 1327 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–	189.538	-63.019	0.459	-7.52	-0.24	-0.781
He et al.	2023	189.535	-63.018	0.455	-7.519	-0.221	-0.78

💡 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–	1.95	3.9	–	708	–	–	–	–
He et al.	2023	1.95	3.90	–	708	–	–	–	–

Visualization

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