CWNU 251

0.00 UTI

0.0

C_N

1.0

C_dens

0.38

C_C3

0.0

C_lit

0.0

C_dup

C3 classification BC

Number of members (P>50%) 22

Radius (P>50% members) 2.4 [arcmin]

C_N 0.0 Sparse
C_dens 1.0 Very dense
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 251 is a sparse, very dense object of low C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, old cluster (see Parameters). It is rarely studied 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 Low extinction Near-solar metallicity Old

Data

🔍 Search references for CWNU 251 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	–	101.974	-7.13	0.413	-0.109	1.784	62.7
He et al.	2022	101.962	-7.128	0.42	-0.11	1.84	68.3

💡 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	2.04	0.60	–	1585	0.169	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 1614	100.0	101.98	-7.13	0.41	-0.11	1.78	62.7	0.46

💡 Note: The % column shows the percentage of members that CWNU 251 shares with each listed object.

Visualization

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