CWNU 1094

0.44 UTI

0.27

C_N

0.92

C_dens

1.0

C_C3

0.0

C_lit

1.0

C_dup

N₅₀ (P>50% members) 27

Stellar density (N₅₀/rad) 4.6 [N/pc²]

C3 classification AA

C_N 0.27 Poorly populated
C_dens 0.92 Very dense
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 1094 is a poorly populated, very dense object of very high C3 quality. Its parallax locates it at a very close distance, near the mid-plane, affected by low extinction. It is catalogued as a young cluster (see Parameters). It is rarely studied in the literature.

Note: This object shares a significant percentage of members with at least one entry reported in the same catalogue. See table with shared members information.

Low extinction Young

Data

🔍 Search references for CWNU 1094 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–	61.662	21.289	8.305	4.192	-14.515	14.995
He et al.	2022	61.487	21.603	8.337	4.321	-14.677	–

💡 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–	–	0.05	–	28	–	–	–	–
He et al.	2022	–	0.05	–	28	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 1340	100.0	68.02	19.84	8.24	0.7	-14.59	15.03	0.25
OCSN 118	100.0	62.83	20.3	8.24	3.7	-13.98	15.09	0.28
CWNU 1108	51.9	63.21	20.39	8.14	3.48	-13.84	15.04	0.3

💡 Note: The % column shows the percentage of members that CWNU 1094 shares with each listed object.

Visualization

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