CWNU 3179

0.18 UTI

0.72

C_N

0.98

C_dens

0.75

C_C3

0.0

C_lit

0.37

C_dup

C3 classification AB

Number of members (P>50%) 95

Radius (P>50% members) 3.2 [arcmin]

C_N 0.72 Moderately populated
C_dens 0.98 Very dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.37 Possibly duplicate

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

Overview

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CWNU 3179 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a young cluster (see Parameters). It was recently reported in the literature.

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

Distant Moderate extinction Young

Data

🔍 Search references for CWNU 3179 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	–	101.089	6.972	0.211	-0.14	-0.547	53.151
He et al.	2023	101.092	6.967	0.207	-0.11	-0.553	–

💡 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.	2023	4.07	1.75	–	25	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Alessi 65	63.2	101.09	6.97	0.21	-0.14	-0.54	53.15	0.46
HSC 1620	54.7	101.09	6.97	0.21	-0.14	-0.54	–	0.01

💡 Note: The % column shows the percentage of members that CWNU 3179 shares with each listed object.

Visualization

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