CWNU 3070

0.29 UTI

0.76

C_N

1.0

C_dens

1.0

C_C3

0.0

C_lit

0.52

C_dup

C3 classification AA

Number of members (P>50%) 133

Radius (P>50% members) 1.4 [arcmin]

C_N 0.76 Rich
C_dens 1.0 Very dense
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 0.52 Likely unique

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

Overview

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CWNU 3070 is a rich, very dense object of very high C3 quality. Its parallax locates it at a large distance, above the mid-plane, affected by very high extinction. It is catalogued as an intermediate-age cluster (see Parameters). It was recently reported in the literature.

Note: This is likely a unique object, which shares a moderate percentage of members with at least one previously reported entry. See table with shared members information.

Very distant Very high extinction Intermediate age

Data

🔍 Search references for CWNU 3070 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	–	263.08	-30.372	0.183	-1.709	-3.036	-205.147
He et al.	2023	263.083	-30.374	0.177	-1.707	-3.035	-84.87

💡 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	5.75	5.95	–	200	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 2966	48.1	263.08	-30.37	0.19	-1.7	-3.02	-82.44	0.61

💡 Note: The % column shows the percentage of members that CWNU 3070 shares with each listed object.

Visualization

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