CWNU 3033

0.03 UTI

0.33

C_N

0.44

C_dens

0.75

C_C3

0.0

C_lit

0.09

C_dup

C3 classification AB

Number of members (P>50%) 33

Radius (P>50% members) 2.1 [arcmin]

C_N 0.33 Poorly populated
C_dens 0.44 Loose
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.09 Very likely duplicate

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

Overview

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CWNU 3033 is a poorly populated, loose object of high C3 quality. Its parallax locates it at a large distance, above the mid-plane, affected by high extinction. It is catalogued as a very young 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.

Very distant High extinction Very young

Data

🔍 Search references for CWNU 3033 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	–	28.774	62.414	0.159	-1.716	0.3	–
He et al.	2023	28.744	62.416	0.16	-1.712	0.279	–

💡 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	6.46	3.65	–	10	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 1053	90.9	28.78	62.41	0.16	-1.71	0.27	–	0.24

💡 Note: The % column shows the percentage of members that CWNU 3033 shares with each listed object.

Visualization

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