CWNU 3045

0.24 UTI

0.75

C_N

1.0

C_dens

0.5

C_C3

0.0

C_lit

0.54

C_dup

C3 classification BB

Number of members (P>50%) 110

Radius (P>50% members) 2.7 [arcmin]

C_N 0.75 Rich
C_dens 1.0 Very dense
C_C3 0.5 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.54 Likely unique

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

Overview

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CWNU 3045 is a rich, very dense object of intermediate C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by high extinction. It is catalogued as a young cluster (see Parameters). It was recently reported in the literature.

Note: This is likely a unique object, which shares a moderate percentage of members with at least one previously reported entry. See table with shared members information.

Very distant High extinction Young

Data

🔍 Search references for CWNU 3045 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	–	132.869	-45.846	0.217	-3.788	4.032	44.086
He et al.	2023	132.875	-45.852	0.208	-3.808	4.043	–

💡 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	6.17	4.80	–	25	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 2141	46.4	132.86	-45.85	0.21	-3.78	4.07	51.21	0.38

💡 Note: The % column shows the percentage of members that CWNU 3045 shares with each listed object.

Visualization

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