CWNU 79

0.07 UTI

0.52

C_N

1.0

C_dens

0.75

C_C3

0.0

C_lit

0.16

C_dup

C3 classification BA

Number of members (P>50%) 55

Radius (P>50% members) 4.0 [arcmin]

C_N 0.52 Moderately populated
C_dens 1.0 Very dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.16 Likely duplicate

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

Overview

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CWNU 79 is a moderately populated, very dense object of high 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, intermediate-age 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 Intermediate age

Data

🔍 Search references for CWNU 79 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	–	113.508	-19.195	0.358	-1.774	2.682	42.265
He et al.	2022	113.501	-19.2	0.36	-1.78	2.66	42.3

💡 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	2.40	1.74	–	631	0.169	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 1378	83.6	113.51	-19.18	0.36	-1.78	2.69	42.43	0.56
UBC 1379	81.8	113.51	-19.19	0.35	-1.77	2.7	42.27	0.44
CWWDL 2073	32.7	113.51	-19.17	0.36	-1.81	2.61	42.59	0.04

💡 Note: The % column shows the percentage of members that CWNU 79 shares with each listed object.

Visualization

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