CWNU 2673

0.07 UTI

0.54

C_N

1.0

C_dens

0.62

C_C3

0.0

C_lit

0.17

C_dup

C3 classification AC

Number of members (P>50%) 58

Radius (P>50% members) 7.4 [arcmin]

C_N 0.54 Moderately populated
C_dens 1.0 Very dense
C_C3 0.62 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.17 Likely duplicate

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

Overview

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CWNU 2673 is a moderately populated, very dense object of intermediate C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by low extinction. It is catalogued as a young cluster (see Parameters). It was recently reported in the literature.

⚠️ Warning: This is 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 Young

Data

🔍 Search references for CWNU 2673 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	–	84.063	34.294	0.749	0.274	-2.364	9.721
He et al.	2023	84.073	34.327	0.749	0.289	-2.369	–

💡 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	1.32	0.90	–	25	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
XDOCC 02	82.8	84.06	34.3	0.75	0.27	-2.36	9.72	0.59

💡 Note: The % column shows the percentage of members that CWNU 2673 shares with each listed object.

Visualization

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