CWNU 179

0.12 UTI

0.62

C_N

1.0

C_dens

1.0

C_C3

0.0

C_lit

0.23

C_dup

C3 classification AA

Number of members (P>50%) 74

Radius (P>50% members) 4.1 [arcmin]

C_N 0.62 Moderately populated
C_dens 1.0 Very dense
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 0.23 Likely duplicate

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

Overview

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CWNU 179 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It is rarely studied in the literature.

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

Relatively close Moderate extinction Near-solar metallicity Young

Data

🔍 Search references for CWNU 179 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	–	270.826	-19.346	0.658	0.052	-1.1	14.541
He et al.	2022	270.841	-19.35	0.64	0.08	-1.11	–

💡 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	1.32	2.52	–	40	0.051	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 1007	77.0	270.82	-19.34	0.66	0.04	-1.09	14.54	0.61
CWWDL 14200	70.3	270.82	-19.35	0.66	0.05	-1.1	14.54	0.0

💡 Note: The % column shows the percentage of members that CWNU 179 shares with each listed object.

Visualization

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