CWNU 3067

0.01 UTI

0.6

C_N

0.91

C_dens

1.0

C_C3

0.0

C_lit

0.03

C_dup

C3 classification AA

Number of members (P>50%) 71

Radius (P>50% members) 3.1 [arcmin]

C_N 0.6 Moderately populated
C_dens 0.91 Very dense
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 0.03 Very likely duplicate

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

Overview

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CWNU 3067 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a moderate^* distance, well above the mid-plane, affected by moderate extinction. It is catalogued as an old cluster (see Parameters). It was recently reported 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.

(*): The parallax distance estimate (~4.39 kpc) differs significantly from the median photometric distance (~3.16 kpc).

Distant Moderate extinction Old

Data

🔍 Search references for CWNU 3067 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	–	71.693	60.877	0.228	0.553	-0.102	-18.761
He et al.	2023	71.689	60.873	0.23	0.559	-0.11	-18.76

💡 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	3.16	1.75	–	1585	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWWDL 3218	97.2	71.69	60.87	0.24	0.55	-0.1	-18.76	0.11
CWWL 3078	88.7	71.69	60.88	0.23	0.55	-0.1	-18.76	0.62

💡 Note: The % column shows the percentage of members that CWNU 3067 shares with each listed object.

Visualization

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