CWNU 2662

0.40 UTI

0.37

C_N

0.89

C_dens

0.75

C_C3

0.0

C_lit

1.0

C_dup

C3 classification BA

Number of members (P>50%) 37

Radius (P>50% members) 2.6 [arcmin]

C_N 0.37 Poorly populated
C_dens 0.89 Dense
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 1.0 Unique

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

Overview

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CWNU 2662 is a poorly populated, dense object of high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by high extinction. It is catalogued as an intermediate-age cluster (see Parameters). It was recently reported in the literature.

Note: This object shares a very small percentage of members with a later reported entry. See table with shared members information.

Distant High extinction Intermediate age

Data

🔍 Search references for CWNU 2662 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	–	281.267	-5.464	0.262	-1.332	-3.197	55.518
He et al.	2023	281.271	-5.471	0.266	-1.326	-3.199	43.62

💡 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	3.24	3.25	–	200	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 273	8.1	281.08	-5.45	0.24	-1.2	-3.1	38.57	0.05

💡 Note: The % column shows the percentage of members that CWNU 2662 shares with each listed object.

Visualization

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