CWNU 3304

0.32 UTI

0.47

C_N

0.39

C_dens

0.75

C_C3

0.0

C_lit

1.0

C_dup

C3 classification AB

Number of members (P>50%) 47

Radius (P>50% members) 2.5 [arcmin]

C_N 0.47 Poorly populated
C_dens 0.39 Loose
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 3304 is a poorly populated, loose object of high C3 quality. Its parallax locates it at a large^* distance, above the mid-plane, affected by low extinction. It is catalogued as an intermediate-age cluster (see Parameters). It was recently reported in the literature.

(*): The parallax distance estimate (~6.79 kpc) differs significantly from the median photometric distance (~4.90 kpc).

Distant Low extinction Intermediate age

Data

🔍 Search references for CWNU 3304 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	–	122.449	-26.489	0.147	-2.018	2.33	58.642
He et al.	2023	122.447	-26.485	0.147	-2.02	2.328	58.64

💡 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	4.90	0.45	–	398	–	–	–	–

Visualization

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