CWNU 3473

0.06 UTI

0.57

C_N

0.56

C_dens

0.75

C_C3

0.0

C_lit

0.17

C_dup

C3 classification AB

Number of members (P>50%) 65

Radius (P>50% members) 1.7 [arcmin]

C_N 0.57 Moderately populated
C_dens 0.56 Moderately dense
C_C3 0.75 High 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 3473 is a moderately populated, moderately dense object of high C3 quality. Its parallax locates it at a large^* distance, well above the mid-plane, affected by moderate extinction. It is catalogued as an intermediate-age 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.

(*): The parallax distance estimate (~9.75 kpc) differs significantly from the median photometric distance (~6.61 kpc).

Very distant Moderate extinction Intermediate age

Data

🔍 Search references for CWNU 3473 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	–	299.026	35.985	0.103	-2.904	-5.055	-3.469
He et al.	2023	299.026	35.986	0.098	-2.914	-5.061	–

💡 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	6.61	1.65	–	794	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
HSC 567	83.1	299.03	35.99	0.1	-2.91	-5.05	-3.47	0.45

💡 Note: The % column shows the percentage of members that CWNU 3473 shares with each listed object.

Visualization

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