CWNU 2970

0.00 UTI

0.27

C_N

0.15

C_dens

0.38

C_C3

0.0

C_lit

0.0

C_dup

C3 classification BC

Number of members (P>50%) 27

Radius (P>50% members) 21.5 [arcmin]

C_N 0.27 Poorly populated
C_dens 0.15 Very loose
C_C3 0.38 Low quality
C_lit 0.0 Rarely studied
C_dup 0.0 Very likely duplicate

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

Overview

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CWNU 2970 is a poorly populated, very loose object of low C3 quality. Its parallax locates it at a close distance, near the mid-plane, affected by moderate extinction. It is catalogued as an intermediate-age 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.

Relatively close Moderate extinction Intermediate age

Data

🔍 Search references for CWNU 2970 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	–	48.868	56.589	1.035	3.132	-2.377	-7.324
He et al.	2023	48.995	56.554	1.024	3.148	-2.387	-17.08

💡 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	1.00	2.15	–	126	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Theia 2482	100.0	48.79	56.6	1.02	3.1	-2.33	-7.32	0.33

💡 Note: The % column shows the percentage of members that CWNU 2970 shares with each listed object.

Visualization

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