CWNU 1192

0.02 UTI

0.0

C_N

0.35

C_dens

0.75

C_C3

0.0

C_lit

0.08

C_dup

N₅₀ (P>50% members) 23

Stellar density (N₅₀/rad) 1.8 [N/pc²]

C3 classification AB

C_N 0.0 Sparse
C_dens 0.35 Loose
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.08 Very likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19

MOCA 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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CWNU 1192 is a sparse, loose object of high C3 quality. Its parallax locates it at a close distance, above the mid-plane, affected by moderate extinction. It is catalogued as a very young 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.

Moderate extinction Very young

Data

🔍 Search references for CWNU 1192 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–	318.535	59.408	1.164	-2.508	-3.496	-25.367
He et al.	2022	318.722	59.333	1.163	-2.502	-3.478	–

💡 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–	–	1.55	–	11	–	–	–	–
He et al.	2022	–	1.55	–	11	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Riddle 6	92.0	318.03	59.9	1.17	-2.53	-3.51	-23.22	0.65
OC 0158	72.0	318.24	59.51	1.16	-2.54	-3.51	-24.65	0.02
UBC 385	8.0	317.94	60.02	1.18	-2.53	-3.51	-17.86	0.0

💡 Note: The % column shows the percentage of members that CWNU 1192 shares with each listed object.

Visualization

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