CWNU 194

0.00 UTI

0.35

C_N

1.0

C_dens

0.62

C_C3

0.0

C_lit

0.0

C_dup

C3 classification CA

Number of members (P>50%) 35

Radius (P>50% members) 2.9 [arcmin]

C_N 0.35 Poorly populated
C_dens 1.0 Very dense
C_C3 0.62 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.0 Very likely duplicate

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

Overview

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CWNU 194 is a poorly populated, very dense object of intermediate C3 quality. Its parallax locates it at a moderate^* distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, old cluster (see Parameters). It is rarely studied in the literature.

⚠️ Warning: This is very likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

(*): The parallax distance estimate (~2.17 kpc) differs significantly from the median photometric distance (~1.66 kpc).

Relatively close Moderate extinction Near-solar metallicity Old

Data

🔍 Search references for CWNU 194 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	–	85.475	29.399	0.462	0.536	-3.526	-11.566
He et al.	2022	85.477	29.396	0.48	0.51	-3.52	-11.1

💡 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.	2022	1.66	2.40	–	1000	-0.082	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 1289	100.0	85.46	29.4	0.46	0.54	-3.53	-11.57	0.56

💡 Note: The % column shows the percentage of members that CWNU 194 shares with each listed object.

Visualization

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